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Pushing the limit of instrument capabilities

Published online by Cambridge University Press:  21 October 2010

Denis V. Shulyak ,
Werner W. Weiss ,
Gautier Mathys ,
Laurent Eyer ,
Alexander F. Kholtygin ,
Oleg Kochukhov ,
Pierre North ,
Sergey N. Fabrika  and
Tatyana E. Burlakova
Denis V. Shulyak
Affiliation:
Institute of Astrophysics, Georg-August-University, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany email: [email protected]
Werner W. Weiss
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstraße 17, 1180 Wien, Austria email: [email protected]
Gautier Mathys
Affiliation:
European Southern Observatory, Casilla 19001, Santiago 19, Chile email: [email protected]
Laurent Eyer
Affiliation:
Observatoire de Genève, 51 ch. des Maillettes, CH-1290 Sauverny, Switzerland email: [email protected]
Alexander F. Kholtygin
Affiliation:
Astronomical Institute, St. Petersburg State University, Universitetskii pr. 28, St. Petersburg, 198504, Russia email: [email protected]
Oleg Kochukhov
Affiliation:
Department of Physics and Astronomy, Uppsala University, Box 515, 751 20, Uppsala, Sweden email: [email protected]
Pierre North
Affiliation:
Ecole Polytechnique Fédérale de Lausanne, 1015 Lausanne, Switzerland email: [email protected]
Sergey N. Fabrika
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Karachai Cherkess Republic, 369167, Russia
Tatyana E. Burlakova
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Karachai Cherkess Republic, 369167, Russia
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Abstract

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Chemically Peculiar (CP) stars have been the subject of systematic research for more than 50 years. With the discovery of pulsation of some of the cool CP stars, and the availability of advanced spectropolarimetric instrumentation and high signal-to-noise, high resolution spectroscopy, a new era of CP star research emerged about 20 years ago. Together with the success in ground-based observations, new space projects are developed that will greatly benefit future investigations of these unique objects. In this contribution we will give an overview of some interesting results obtained recently from ground-based observations and discuss the future outstanding Gaia space mission and its impact on CP star research.

Keywords

stars: chemically peculiarstars: atmospheresstars: variables: roApstars: oscillationsspace vehicles: instrumentsGaia mission
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 142 - 150
Copyright
Copyright © International Astronomical Union 2010

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