F7601 Physics of hot stars

Faculty of Science
Spring 2023
Extent and Intensity
2/0/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Timetable
Thu 10:00–11:50 Fs1 6/1017
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Learning outcomes
The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021.

F7601 Physics of hot stars

Faculty of Science
Spring 2021
Extent and Intensity
2/0/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Timetable
Mon 1. 3. to Fri 14. 5. Mon 13:00–14:50 online_F4
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Learning outcomes
The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
Study Materials
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2019
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Jana Musilová, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Timetable
Mon 18. 2. to Fri 17. 5. Mon 13:00–14:50 F3,03015
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
Study Materials
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2017
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Jana Musilová, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Timetable
Mon 20. 2. to Mon 22. 5. Thu 14:00–15:50 FLenc,03028
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
Study Materials
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2015
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Timetable
Tue 12:00–13:50 F3,03015
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2013
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Timetable
Thu 17:00–18:50 Fs1 6/1017
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2011
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Timetable
Mon 11:00–12:50 F4,03017
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
Study Materials
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2009
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Timetable
Mon 12:00–13:50 F3,03015
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2007
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Timetable
Fri 8:00–9:50 F3,03015
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives (in Czech)
Předmět představuje úvod do problematiky studia hvězd raných spektrálních typů a hvězdných soustav s horkými složkami. Téma je shodě se zaměřením astronomické skupiny pracovníků Ústavu teoretické fyziky a astrofyziky PřF MU.
Syllabus (in Czech)
  • Definice horkých hvězd. Základní charakteristiky - hmotnosti, teploty, zářivé výkony, zastoupení ve hvězdné populaci, rozložení v Galaxii. HR diagram horkých hvězd a jeho výklad. Vnitřní stavba. Vývojový status (opakování stavby a vývoje hvězd). Dvojhvězdy a vícenásobné hvězdné systémy s horkými složkami. Role horkých hvězd ve vývoji Galaxie. Spektroskopická a fotometrická diagnostika horkých hvězd. Proměnnost horkých hvězd - pulzační: delta Sct, beta Cep, ZZ Cet Chemicky pekuliární hvězdy raných spektrálních tříd. Be hvězdy. Hvězdný vítr.
Assessment methods (in Czech)
2 hodiny klasických přednášek. V případě zájmu budou i konzultace. Při zkoušce si zkoušený vylosuje otázku a má 60 minut na přípravu, během níž může používat libovolné pomůcky včetně vlastních poznámek a skript. Vlastní zkouška, jež trvá 30 minut, je individuální a poměrně náročná, jejím cílem je zjistit do jaké míry zkoušený učivu porozuměl.
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2005
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Michal Lenc, Ph.D.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Timetable
Fri 8:00–9:50 F2-8
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives (in Czech)
Předmět představuje úvod do problematiky studia hvězd raných spektrálních typů a hvězdných soustav s horkými složkami. Téma je shodě se zaměřením astronomické skupiny pracovníků Ústavu teoretické fyziky a astrofyziky PřF MU.
Syllabus (in Czech)
  • Definice horkých hvězd. Základní charakteristiky - hmotnosti, teploty, zářivé výkony, zastoupení ve hvězdné populaci, rozložení v Galaxii. HR diagram horkých hvězd a jeho výklad. Vnitřní stavba. Vývojový status (opakování stavby a vývoje hvězd). Dvojhvězdy a vícenásobné hvězdné systémy s horkými složkami. Role horkých hvězd ve vývoji Galaxie. Spektroskopická a fotometrická diagnostika horkých hvězd. Proměnnost horkých hvězd - pulzační: delta Sct, beta Cep, ZZ Cet Chemicky pekuliární hvězdy raných spektrálních tříd. Be hvězdy. Hvězdný vítr.
Assessment methods (in Czech)
2 hodiny klasických přednášek. V případě zájmu budou i konzultace. Při zkoušce si zkoušený vylosuje otázku a má 60 minut na přípravu, během níž může používat libovolné pomůcky včetně vlastních poznámek a skript. Vlastní zkouška, jež trvá 30 minut, je individuální a poměrně náročná, jejím cílem je zjistit do jaké míry zkoušený učivu porozuměl.
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2003
Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Michal Lenc, Ph.D.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives (in Czech)
Předmět představuje úvod do problematiky studia hvězd raných spektrálních typů a hvězdných soustav s horkými složkami. Téma je shodě se zaměřením astronomické skupiny pracovníků Ústavu teoretické fyziky a astrofyziky PřF MU.
Syllabus (in Czech)
  • Definice horkých hvězd. Základní charakteristiky - hmotnosti, teploty, zářivé výkony, zastoupení ve hvězdné populaci, rozložení v Galaxii. HR diagram horkých hvězd a jeho výklad. Vnitřní stavba. Vývojový status (opakování stavby a vývoje hvězd). Dvojhvězdy a vícenásobné hvězdné systémy s horkými složkami. Role horkých hvězd ve vývoji Galaxie. Spektroskopická a fotometrická diagnostika horkých hvězd. Proměnnost horkých hvězd - pulzační: delta Sct, beta Cep, ZZ Cet Chemicky pekuliární hvězdy raných spektrálních tříd. Be hvězdy. Hvězdný vítr.
Assessment methods (in Czech)
2 hodiny klasických přednášek. V případě zájmu budou i konzultace. Při zkoušce si zkoušený vylosuje otázku a má 60 minut na přípravu, během níž může používat libovolné pomůcky včetně vlastních poznámek a skript. Vlastní zkouška, jež trvá 30 minut, je individuální a poměrně náročná, jejím cílem je zjistit do jaké míry zkoušený učivu porozuměl.
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2024

The course is not taught in Spring 2024

Extent and Intensity
2/0/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Learning outcomes
The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2022

The course is not taught in Spring 2022

Extent and Intensity
2/0/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Learning outcomes
The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2020

The course is not taught in Spring 2020

Extent and Intensity
2/0/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Learning outcomes
The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
spring 2018

The course is not taught in spring 2018

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Jana Musilová, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2016

The course is not taught in Spring 2016

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Jana Musilová, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2014

The course is not taught in Spring 2014

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2012

The course is not taught in Spring 2012

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2010

The course is not taught in Spring 2010

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2008

The course is not taught in Spring 2008

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives (in Czech)
Předmět představuje úvod do problematiky studia hvězd raných spektrálních typů a hvězdných soustav s horkými složkami. Téma je shodě se zaměřením astronomické skupiny pracovníků Ústavu teoretické fyziky a astrofyziky PřF MU.
Syllabus (in Czech)
  • Definice horkých hvězd. Základní charakteristiky - hmotnosti, teploty, zářivé výkony, zastoupení ve hvězdné populaci, rozložení v Galaxii. HR diagram horkých hvězd a jeho výklad. Vnitřní stavba. Vývojový status (opakování stavby a vývoje hvězd). Dvojhvězdy a vícenásobné hvězdné systémy s horkými složkami. Role horkých hvězd ve vývoji Galaxie. Spektroskopická a fotometrická diagnostika horkých hvězd. Proměnnost horkých hvězd - pulzační: delta Sct, beta Cep, ZZ Cet Chemicky pekuliární hvězdy raných spektrálních tříd. Be hvězdy. Hvězdný vítr.
Assessment methods (in Czech)
2 hodiny klasických přednášek. V případě zájmu budou i konzultace. Při zkoušce si zkoušený vylosuje otázku a má 60 minut na přípravu, během níž může používat libovolné pomůcky včetně vlastních poznámek a skript. Vlastní zkouška, jež trvá 30 minut, je individuální a poměrně náročná, jejím cílem je zjistit do jaké míry zkoušený učivu porozuměl.
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2006

The course is not taught in Spring 2006

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Michal Lenc, Ph.D.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives (in Czech)
Předmět představuje úvod do problematiky studia hvězd raných spektrálních typů a hvězdných soustav s horkými složkami. Téma je shodě se zaměřením astronomické skupiny pracovníků Ústavu teoretické fyziky a astrofyziky PřF MU.
Syllabus (in Czech)
  • Definice horkých hvězd. Základní charakteristiky - hmotnosti, teploty, zářivé výkony, zastoupení ve hvězdné populaci, rozložení v Galaxii. HR diagram horkých hvězd a jeho výklad. Vnitřní stavba. Vývojový status (opakování stavby a vývoje hvězd). Dvojhvězdy a vícenásobné hvězdné systémy s horkými složkami. Role horkých hvězd ve vývoji Galaxie. Spektroskopická a fotometrická diagnostika horkých hvězd. Proměnnost horkých hvězd - pulzační: delta Sct, beta Cep, ZZ Cet Chemicky pekuliární hvězdy raných spektrálních tříd. Be hvězdy. Hvězdný vítr.
Assessment methods (in Czech)
2 hodiny klasických přednášek. V případě zájmu budou i konzultace. Při zkoušce si zkoušený vylosuje otázku a má 60 minut na přípravu, během níž může používat libovolné pomůcky včetně vlastních poznámek a skript. Vlastní zkouška, jež trvá 30 minut, je individuální a poměrně náročná, jejím cílem je zjistit do jaké míry zkoušený učivu porozuměl.
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2004

The course is not taught in Spring 2004

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Michal Lenc, Ph.D.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives (in Czech)
Předmět představuje úvod do problematiky studia hvězd raných spektrálních typů a hvězdných soustav s horkými složkami. Téma je shodě se zaměřením astronomické skupiny pracovníků Ústavu teoretické fyziky a astrofyziky PřF MU.
Syllabus (in Czech)
  • Definice horkých hvězd. Základní charakteristiky - hmotnosti, teploty, zářivé výkony, zastoupení ve hvězdné populaci, rozložení v Galaxii. HR diagram horkých hvězd a jeho výklad. Vnitřní stavba. Vývojový status (opakování stavby a vývoje hvězd). Dvojhvězdy a vícenásobné hvězdné systémy s horkými složkami. Role horkých hvězd ve vývoji Galaxie. Spektroskopická a fotometrická diagnostika horkých hvězd. Proměnnost horkých hvězd - pulzační: delta Sct, beta Cep, ZZ Cet Chemicky pekuliární hvězdy raných spektrálních tříd. Be hvězdy. Hvězdný vítr.
Assessment methods (in Czech)
2 hodiny klasických přednášek. V případě zájmu budou i konzultace. Při zkoušce si zkoušený vylosuje otázku a má 60 minut na přípravu, během níž může používat libovolné pomůcky včetně vlastních poznámek a skript. Vlastní zkouška, jež trvá 30 minut, je individuální a poměrně náročná, jejím cílem je zjistit do jaké míry zkoušený učivu porozuměl.
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
spring 2012 - acreditation

The information about the term spring 2012 - acreditation is not made public

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Supplier department: Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2011 - only for the accreditation

The course is not taught in Spring 2011 - only for the accreditation

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives
The course is an introduction to the study of early type stars and binaries with early type components. The topic corresponds to the research field of a group of members of the Department of Theoretical Physics and Astrophysics. The students obtain information that allows them to do research work in the field of early type stars.
Syllabus
  • Definition of hot stars
  • Main characteristics - mass, temperature, luminosity, population membership, distribution in Galaxy
  • HR diagram of hot stars and its explanation
  • Inner structure
  • Evolutionary status (repetition of stellar structure and evolution).
  • Binaries and multiple systems with hot components
  • Role of hot stars in the Galaxy evolution.
  • Spectroscopic and photometric analysis of hot stars.
  • Variability of hot stars - pulsations: delta Sct, beta Cep, ZZ Cet
  • Early type chemically peculiar stars
  • Be stars
  • Stellar wind
Literature
  • MIKULÁŠEK, Zdeněk and Jiří KRTIČKA. Fyzika horkých hvězd. 2007. URL info
  • KIPPENHAHN, Rudolf and Alfred WEIGERT. Stellar structure and evolution. 3rd corr. print. Berlin: Springer-Verlag, 1994, xvi, 468 s. ISBN 3-540-58013-1-. info
  • An introduction to modern astrophysics. Edited by Bradley W. Carroll - Dale A. Ostlie. 2nd ed. San Francisco: Pearson Addison-Wesley, 2007, 1 v. (vari. ISBN 978-0-321-44284-0. info
  • LAMERS, Henny J. G. L. M. and Joseph P. CASSINELLI. Introduction to stellar winds. 1st pub. Cambridge: Cambridge University Press, 1999, xiv, 438. ISBN 0521593980. info
  • KRTIČKA, Jiří, Daniela KORČÁKOVÁ and Jiří KUBÁT. Challenges to the theories of B stars circumstellar environment. In Publ. Astron. Inst. Czech. 93rd ed. Ondrejov: AsU AV CR, 2005, p. 29-35. URL info
  • KRTIČKA, Jiří and Jiří KUBÁT. Radiatively Driven Winds of OB Stars - from Micro to Macro (Radiatively Driven Winds of OB Stars -- from Micro to Macro). In Active OB-Stars: Laboratories For Stellar and Circumstellar Physics. San Francisco, USA: Astronomical Society of the Pacific, 2007, p. 153-164. ISBN 978-1-583812-29-7. URL info
Teaching methods
Lectures
Assessment methods
2 hours of lectures per week, oral exam, it is possible to use any literature during the exam
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.

F7601 Physics of hot stars

Faculty of Science
Spring 2008 - for the purpose of the accreditation

The course is not taught in Spring 2008 - for the purpose of the accreditation

Extent and Intensity
2/0. 1 credit(s) (fasci plus compl plus > 4). Type of Completion: zk (examination).
Teacher(s)
prof. RNDr. Zdeněk Mikulášek, CSc. (lecturer)
prof. Mgr. Jiří Krtička, Ph.D. (lecturer)
Guaranteed by
prof. RNDr. Zdeněk Mikulášek, CSc.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Zdeněk Mikulášek, CSc.
Prerequisites
The graduation of the courses "An introduction to stellar physics", "An introduction into physics of stellar systems" and "The physics of stellar atmospheres" is strongly recommended.
Course Enrolment Limitations
The course is offered to students of any study field.
Course objectives (in Czech)
Předmět představuje úvod do problematiky studia hvězd raných spektrálních typů a hvězdných soustav s horkými složkami. Téma je shodě se zaměřením astronomické skupiny pracovníků Ústavu teoretické fyziky a astrofyziky PřF MU.
Syllabus (in Czech)
  • Definice horkých hvězd. Základní charakteristiky - hmotnosti, teploty, zářivé výkony, zastoupení ve hvězdné populaci, rozložení v Galaxii. HR diagram horkých hvězd a jeho výklad. Vnitřní stavba. Vývojový status (opakování stavby a vývoje hvězd). Dvojhvězdy a vícenásobné hvězdné systémy s horkými složkami. Role horkých hvězd ve vývoji Galaxie. Spektroskopická a fotometrická diagnostika horkých hvězd. Proměnnost horkých hvězd - pulzační: delta Sct, beta Cep, ZZ Cet Chemicky pekuliární hvězdy raných spektrálních tříd. Be hvězdy. Hvězdný vítr.
Assessment methods (in Czech)
2 hodiny klasických přednášek. V případě zájmu budou i konzultace. Při zkoušce si zkoušený vylosuje otázku a má 60 minut na přípravu, během níž může používat libovolné pomůcky včetně vlastních poznámek a skript. Vlastní zkouška, jež trvá 30 minut, je individuální a poměrně náročná, jejím cílem je zjistit do jaké míry zkoušený učivu porozuměl.
Language of instruction
Czech
Further comments (probably available only in Czech)
The course is taught once in two years.
The course is taught: every week.
General note: S.
The course is also listed under the following terms Spring 2003, Spring 2005, Spring 2007, Spring 2009, Spring 2011, spring 2012 - acreditation, Spring 2013, Spring 2015, Spring 2017, Spring 2019, Spring 2021, Spring 2023.
  • Enrolment Statistics (recent)