000002842 001__ 2842
000002842 005__ 20160701171711.0
000002842 0247_ $$2DOI$$a10.1051/eas/1045062
000002842 037__ $$aASTROimport-999
000002842 100__ $$aBlomme, R.
000002842 245__ $$aEmission-line Stars and Early-type Stars with Gaia
000002842 260__ $$c2011
000002842 520__ $$aGaia will provide accurate parallaxes, spectrophotometry and spectroscopy for hundreds of thousands of emission-line stars across the whole HR diagram. In preparation for the Gaia mission, we are developing algorithms to recognize and classify emission-line stars. A large collection of ground-based spectroscopic observations has been collected and will be used for testing and training the algorithms. Gaia will also provide information on several millions of early-type stars. Determining accurate parameters for these stars from Gaia data only will be difficult due to the AV - Teff degeneracy. 
000002842 700__ $$a Frémat, Y.
000002842 700__ $$a Lobel, A.
000002842 700__ $$a Martayan, C.
000002842 773__ $$c373-376$$pEAS Publications Series$$v45$$y2011
000002842 85642 $$ahttp://esoads.eso.org/abs/2011EAS....45..373B
000002842 905__ $$apublished in
000002842 980__ $$aNONREF