F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of Sciencespring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of Sciencespring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
F7601 Physics of hot stars
Faculty of ScienceSpring 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.
- Enrolment Statistics (recent)