000002556 001__ 2556
000002556 005__ 20160701171707.0
000002556 037__ $$aASTROimport-713
000002556 100__ $$aGutiérrez-Soto, J.
000002556 245__ $$aFirst results on Be stars with CoRoT
000002556 260__ $$c2008
000002556 520__ $$aIn this paper we present an overview of the analysis of some of the Be stars observed with the CoRoT satellite up to this date. Be stars are very fast-rotating B-type stars which may pulsate as ß Cephei or SPB stars. CoRoT has already observed 5 bright Be stars in the seismology fields and several tens of fainter ones in the exoplanet fields with an unprecedented quality and with a time duration from 20 to 150 days. Multiple frequencies are detected in the majority of the stars. Pulsations, outbursts, beating phenomenon, rotation, amplitude variability, etc. have been found in their light curves. In order to complement this study, ground-based spectroscopic data have also been analysed for the stars located in the seismology fields. 
000002556 700__ $$a Neiner, C.
000002556 700__ $$a Hubert, A.-M.
000002556 700__ $$a Floquet, M.
000002556 700__ $$a Huat, A.-L.
000002556 700__ $$a Diago, P. D.
000002556 700__ $$a Fabregat, J.
000002556 700__ $$a Leroy, B.
000002556 700__ $$a de Batz, B.
000002556 700__ $$a Andrade, L.
000002556 700__ $$a Emilio, M.
000002556 700__ $$a Facanha, W.
000002556 700__ $$a Frémat, Y.
000002556 700__ $$a Janot-Pacheco, E.
000002556 700__ $$a Martayan, M.
000002556 700__ $$a Suso, J.
000002556 700__ $$a Garrido, R.
000002556 773__ $$c475$$pSF2A-2008$$y2008
000002556 85642 $$ahttp://esoads.eso.org/abs/2008sf2a.conf..475G
000002556 905__ $$apublished in
000002556 980__ $$aNONREF