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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.
Om dit artikel te citeren:
Over : Yassine Damerdji
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Over : Ludovic Delchambre
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Over : Thierry Morel
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Over : Eric Gosset
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Over : Gregor Rauw
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium