Reference : The Gaia satellite: a tool for Emission Line Stars and Hot Stars
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/15928
The Gaia satellite: a tool for Emission Line Stars and Hot Stars
English
Martayan, C. [> > > >]
Frémat, Y. [> > > >]
Blomme, R. [> > > >]
Jonckheere, A. [> > > >]
Borges, M. [> > > >]
de Batz, B. [> > > >]
Leroy, B. [ > > ]
Sordo, R. [> > > >]
Bouret, J.-C. [> > > >]
Martins, F. [> > > >]
Zorec, J. [> > > >]
Neiner, C. [> > > >]
Nazé, Yaël mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Sciences spatiales >]
Alecian, E. [> > > >]
Floquet, M. [> > > >]
Hubert, A.-M. [> > > >]
Briot, D. [> > > >]
Miroshnichenko, A. [> > > >]
Kolka, I. [> > > >]
Stee, P. [ > > ]
Lanz, T. [> > > >]
Meynet, G. [> > > >]
1-Nov-2008
SF2A-2008
499
No
International
[en] The 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.
Professionals
http://hdl.handle.net/2268/15928
http://arxiv.org/abs/0809.4417
http://adsabs.harvard.edu/abs/2008sf2a.conf..499M

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