000002323 001__ 2323
000002323 005__ 20160701171703.0
000002323 037__ $$aASTROimport-480
000002323 100__ $$aNeiner, C.
000002323 245__ $$aPreliminary results on the pulsations of Be stars with CoRoT
000002323 260__ $$c2009
000002323 520__ $$aWe present preliminary results of the study of pulsations of Be stars from CoRoT observations. CoRoT detected many pulsation frequencies in all observed Be stars, usually interpreted in terms of g-modes but sometimes also corresponding to p-modes. Even in late Be stars, for which the detection of pulsation frequencies is very difficult from the ground, because of their very low amplitude, the quality and precision of the CoRoT data allows us to detect many frequencies. Seismic models have not yet been calculated but the calculations are ongoing. 
000002323 700__ $$a Gutiérrez-Soto, J.
000002323 700__ $$a Floquet, M.
000002323 700__ $$a Huat, A.-L.
000002323 700__ $$a Hubert, A.-M.
000002323 700__ $$a de Batz, B.
000002323 700__ $$a Leroy, B.
000002323 700__ $$a Frémat, Y.
000002323 700__ $$a Andrade, L.
000002323 700__ $$a Diago, P. D.
000002323 700__ $$a Emilio, M.
000002323 700__ $$a Fabregat, J.
000002323 700__ $$a Janot-Pacheco, E.
000002323 700__ $$a Martayan, C.
000002323 700__ $$a Semaan, T.
000002323 700__ $$a Suso, J.
000002323 773__ $$c319$$pCommunications in Asteroseismology$$v158$$y2009
000002323 85642 $$ahttp://esoads.eso.org/abs/2009CoAst.158..319N
000002323 905__ $$apublished in
000002323 980__ $$aREFERD