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A 3-D look into the atmosphere?

Published online by Cambridge University Press:  21 October 2010

G. A. Wade ,
L. Mashonkina ,
T. Ryabchikova ,
J. Krticka ,
J. Silvester ,
O. Kochukhov ,
J. C. Sousa ,
T. Nomura ,
G. M. Wahlgren  and
M. Gruberbauer
...Show all authors
G. A. Wade
Affiliation:
Royal Military College, Canada
L. Mashonkina
Affiliation:
Institute of Astronomy, Russian Academy of Sciences, Russia
T. Ryabchikova
Affiliation:
Institute of Astronomy, Russian Academy of Sciences, Russia
J. Krticka
Affiliation:
Masaryk University, Czech Republic
J. Silvester
Affiliation:
Royal Military College, Canada
O. Kochukhov
Affiliation:
Uppsala University, Sweden
J. C. Sousa
Affiliation:
CAUP-Centro de Astrofisica da Universidade do Porto, Portugal
T. Nomura
Affiliation:
University of Tokyo, Japan
G. M. Wahlgren
Affiliation:
NASA-GSFC/CUA, USA
M. Gruberbauer
Affiliation:
St Mary's University, Canada
S. Hubrig
Affiliation:
Astrophysikalisches Institut Potsdam, Germany
M. Briquet
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium
K. Yüce
Affiliation:
Ankara University, Turkey
N. Drake
Affiliation:
Sobolev Astronomical Institute of St. Petersburg State University, Russia
N. Nunez
Affiliation:
Casleo-UNSJ, Argentina
R. O. Gray
Affiliation:
Appalachian State University, USA
J. Ziznovsky
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, Slovakia
C. Cowley
Affiliation:
Dep. of Astronomy, University of Michigan, USA
A. Shavrina
Affiliation:
Main Astronomical Observatory, National Academy of Sciences of Ukraine
M. Dworetsky
Affiliation:
University College London, United Kingdom
O. Pintado
Affiliation:
Instituto Superior de Correlación Geológica-CONICET, Argentina
N. Polosukhina
Affiliation:
Crimean Astrophysical Observatory, Ukraine
L. Cidale
Affiliation:
Faculdad de Ciencias Astronomicas y Geofisicas, Argentina
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Abstract

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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”.

Keywords

stars: chemically peculiarstars: atmospheresstars: variables: roAp starsstars: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 151 - 160
Copyright
Copyright © International Astronomical Union 2010

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