Spectroscopic binaries as observed by the future Gaia space mission

Yassine Damerdji; Ludovic Delchambre; Thierry Morel; Eric Gosset; Gregor Rauw

Bulletin de la Société Royale des Sciences de Liège

0037-9565 1783-5720

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sinds 05 februari 2011 :
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Yassine Damerdji, Ludovic Delchambre, Thierry Morel, Eric Gosset & Gregor Rauw

Spectroscopic binaries as observed by the future Gaia space mission

(Volume 80 - Année 2011)

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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:

Yassine Damerdji, Ludovic Delchambre, Thierry Morel, Eric Gosset & Gregor Rauw, «Spectroscopic binaries as observed by the future Gaia space mission», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 80 - Année 2011, 481 - 485 URL : http://popups.ulg.be/0037-9565/index.php?id=2970.