The Gaia satellite: a tool for Emission Line Stars and Hot Stars

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dc.creatorMartayan, Christophe
dc.creatorFremat, Yves
dc.creatorBlomme, Ronny
dc.creatorJonckheere, Anthony
dc.creatorBorges, Marcelo
dc.creatorDe Batz, Bertrand
dc.creatorLeroy, Bernard
dc.creatorSordo, Rosanna
dc.creatorBouret, Jean-Claude
dc.creatorMartins, Fabrice
dc.creatorZorec, Jean
dc.creatorNeiner, Coralie
dc.creatorNazé, Yael
dc.creatorAlecian, Evelyne
dc.creatorFloquet, Michele
dc.creatorHubert, Anne-Marie
dc.creatorBriot, Danielle
dc.creatorMiroshnichenko, Anatholy
dc.creatorKolka, Indrek
dc.creatorStee, Philippe
dc.creatorLanz, Thierry
dc.creatorMeynet, Georges
dc.date2008-09-25
dc.date.accessioned2026-07-07T10:05:18Z
dc.date.available2026-07-07T10:05:18Z
dc.descriptionThe Gaia satellite will be launched at the end of 2011. It will observe at least 1 billion stars, and among them several million emission line stars and hot stars. Gaia will provide parallaxes for each star and spectra for stars till V magnitude equal to 17. After a general description of Gaia, we present the codes and methods, which are currently developed by our team. They will provide automatically the astrophysical parameters and spectral classification for the hot and emission line stars in the Milky Way and other close Local Group galaxies such as the Magellanic Clouds.
dc.descriptionSF2A2008, session GAIA, invited talk
dc.identifierhttps://arxiv.org/abs/0809.4417
dc.identifierhttp://arxiv.org/abs/0809.4417
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/169971
dc.subjectAstrophysics
dc.titleThe Gaia satellite: a tool for Emission Line Stars and Hot Stars
dc.typetext

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