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- Volume 80 - Année 2011
- Spectroscopic binaries as observed by the future Gaia space mission
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Spectroscopic binaries as observed by the future Gaia space mission
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Abstract
The future Gaia satellite will observe a large number of stars through its three main channels: astrometric, photometric and, for the brightest stars, spectroscopic. The satellite is equipped with the RVS spectrograph, which will provide medium-resolution spectra over a small wavelength range. These spectra should allow us to identify stars exhibiting a composite spectrum, either because of a chance alignment or a true binarity. We discuss the various aspects related to the data treatment of the binary candidates and describe the algorithms that are intended to be included in the processing pipeline.
Para citar este artículo
Acerca de: Yassine Damerdji
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Acerca de: Ludovic Delchambre
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Acerca de: Thierry Morel
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Acerca de: Eric Gosset
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Acerca de: Gregor Rauw
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium