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.
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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
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW 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
Tags AKb, rivok
Tags International impact
Changed by Changed by: Ing. Andrea Mikešková, učo 137293. Changed: 20/4/2012 12:15.
Abstract
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".
Abstract (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 projectName: 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
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