A 3-D look into the atmosphere?

D 2010

A 3-D look into the atmosphere?

WADE, GA., L. MASHONKINA, T. RYABCHIKOVA, Jiří KRTIČKA, J. SILVESTER et. al.

Basic information

Original name

A 3-D look into the atmosphere?

Name in Czech

3D pohled do atmosféry?

Authors

WADE, GA. (124 Canada), L. MASHONKINA (643 Russian Federation), T. RYABCHIKOVA (643 Russian Federation), Jiří KRTIČKA (203 Czech Republic, guarantor, belonging to the institution), J. SILVESTER (124 Canada), O. KOCHUKHOV (752 Sweden), JC. SOUSA (620 Portugal), T. NOMURA (392 Japan), GM. WAHLGREN (840 United States of America), M. GRUBERBAUER (124 Canada), S. HUBRIG (276 Germany), M. BRIQUET (56 Belgium), K. YUCE (792 Turkey), N. DRAKE (643 Russian Federation), N. NUNEZ (32 Argentina), RO. GRAY (840 United States of America), Jozef ŽIŽNOVSKÝ (703 Slovakia, belonging to the institution), C. COWLEY (840 United States of America), A. SHAVRINA (643 Russian Federation), M. DWORETSKY (826 United Kingdom of Great Britain and Northern Ireland), O. PINTADO (32 Argentina), N. POLOSUKHINA (643 Russian Federation) and L. CIDALE (32 Argentina)

Edition

Cambridge, Highlights of Astronomy, p. 151-160, 10 pp. 2010

Publisher

IAU

Other information

Language

English

Type of outcome

Stať ve sborníku

Field of Study

10308 Astronomy

Country of publisher

United Kingdom of Great Britain and Northern Ireland

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

URL

RIV identification code

RIV/00216224:14310/10:00049542

Organization unit

Faculty of Science

ISBN

978-1-107-00533-4

DOI

http://dx.doi.org/10.1017/S1743921310008550

UT WoS

000290186900042

Keywords (in Czech)

hvězdy: chemicky pekuliární atmosféry proměnné

Keywords in English

stars: chemically peculiar stars: atmospheres stars: variables: roAp stars stars: magnetic fields

Abstract

ORIG CZ

V originále

The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In addition to providing an important window to understanding the physical processes at play in these complex atmospheres, they can also be exploited to study stellar pulsations. This article reviews contributions to the session "A 3D look into the atmosphere" of the Joint Discussion "Progress in understanding the physics of Ap and related stars". It is divided into 3 sections: "Magnetic field and surface structures", "Pulsations in the atmospheres of roAp stars/inversions", and "Spectral synthesis/atmospheric models".

In Czech

Atmosféry chemicky pekuliárních hvězd jsou podstatným způsobem strukturované, a to jak horizontálně, tak vertikálne. Ačkoliv jsou tyto struktury podstatné zejména pro magnetické hvězdy, existují i u hvězd nemagnetických. Tento článek je přehledový, shrnuje příspěvky setkání "Progress in understanding the physics of Ap and related stars".

Links

IAA301630901, research and development project

Name: Rozložení energie ve spektru horkých hvězd a jeho proměnnost

Investor: Academy of Sciences of the Czech Republic, Spectral energy distribution of hot stars and its variability

Citovat

WADE, GA., L. MASHONKINA, T. RYABCHIKOVA, Jiří KRTIČKA, J. SILVESTER, O. KOCHUKHOV, JC. SOUSA, T. NOMURA, GM. WAHLGREN, M. GRUBERBAUER, S. HUBRIG, M. BRIQUET, K. YUCE, N. DRAKE, N. NUNEZ, RO. GRAY, Jozef ŽIŽNOVSKÝ, C. COWLEY, A. SHAVRINA, M. DWORETSKY, O. PINTADO, N. POLOSUKHINA and L. CIDALE. A 3-D look into the atmosphere? In Highlights of Astronomy. Cambridge: IAU, 2010, p. 151-160. ISBN 978-1-107-00533-4. Available from: https://dx.doi.org/10.1017/S1743921310008550.

@inproceedings{975349,
   author = {Wade, GA. and Mashonkina, L. and Ryabchikova, T. and Krtička, Jiří and Silvester, J. and Kochukhov, O. and Sousa, JC. and Nomura, T. and Wahlgren, GM. and Gruberbauer, M. and Hubrig, S. and Briquet, M. and Yuce, K. and Drake, N. and Nunez, N. and Gray, RO. and Žižnovský, Jozef and Cowley, C. and Shavrina, A. and Dworetsky, M. and Pintado, O. and Polosukhina, N. and Cidale, L.},
   address = {Cambridge},
   booktitle = {Highlights of Astronomy},
   doi = {http://dx.doi.org/10.1017/S1743921310008550},
   keywords = {stars: chemically peculiar stars: atmospheres stars: variables: roAp stars stars: magnetic fields},
   language = {eng},
   location = {Cambridge},
   isbn = {978-1-107-00533-4},
   pages = {151-160},
   publisher = {IAU},
   title = {A 3-D look into the atmosphere?},
   url = {http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=7915275},
   year = {2010}
}

TY  - JOUR
ID  - 975349
AU  - Wade, GA. - Mashonkina, L. - Ryabchikova, T. - Krtička, Jiří - Silvester, J. - Kochukhov, O. - Sousa, JC. - Nomura, T. - Wahlgren, GM. - Gruberbauer, M. - Hubrig, S. - Briquet, M. - Yuce, K. - Drake, N. - Nunez, N. - Gray, RO. - Žižnovský, Jozef - Cowley, C. - Shavrina, A. - Dworetsky, M. - Pintado, O. - Polosukhina, N. - Cidale, L.
PY  - 2010
TI  - A 3-D look into the atmosphere?
PB  - IAU
CY  - Cambridge
SN  - 9781107005334
KW  - stars: chemically peculiar stars: atmospheres stars: variables: roAp stars stars: magnetic fields
UR  - http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=7915275
L2  - http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=7915275
N2  - The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In addition to providing an important window to understanding the physical processes at play in these complex atmospheres, they can also be exploited to study stellar pulsations. This article reviews contributions to the session "A 3D look into the atmosphere" of the Joint Discussion "Progress in understanding the physics of Ap and related stars". It is divided into 3 sections: "Magnetic field and surface structures", "Pulsations in the atmospheres of roAp stars/inversions", and "Spectral synthesis/atmospheric models".
ER  -

WADE, GA., L. MASHONKINA, T. RYABCHIKOVA, Jiří KRTIČKA, J. SILVESTER, O. KOCHUKHOV, JC. SOUSA, T. NOMURA, GM. WAHLGREN, M. GRUBERBAUER, S. HUBRIG, M. BRIQUET, K. YUCE, N. DRAKE, N. NUNEZ, RO. GRAY, Jozef ŽIŽNOVSKÝ, C. COWLEY, A. SHAVRINA, M. DWORETSKY, O. PINTADO, N. POLOSUKHINA and L. CIDALE. A 3-D look into the atmosphere? In \textit{Highlights of Astronomy}. Cambridge: IAU, 2010, p.~151-160. ISBN~978-1-107-00533-4. Available from: https://dx.doi.org/10.1017/S1743921310008550.

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