The B0.5IVe CoRoT target HD 49330*

Authors :: Huat, A.-L.
Hubert, A.-M.
Baudin, F.
Floquet, M.
Neiner, C.
Frémat, Y.
Gutiérrez-Soto, J.
Andrade, L.
de Batz, B.
Diago, P. D.
Emilio, M.
Espinosa Lara, F.
Fabregat, J.
Janot-Pacheco, E.
Leroy, B.
Martayan, C.
Semaan, T.
Suso, J.
Auvergne, M.
Catala, C.
Michel, E.
Samadi, R.
Huat, A.-L.
Hubert, A.-M.
Baudin, F.
Floquet, M.
Neiner, C.
Frémat, Y.
Gutiérrez-Soto, J.
Andrade, L.
de Batz, B.
Diago, P. D.
Emilio, M.
Espinosa Lara, F.
Fabregat, J.
Janot-Pacheco, E.
Leroy, B.
Martayan, C.
Semaan, T.
Suso, J.
Auvergne, M.
Catala, C.
Michel, E.
Samadi, R.
Source :: Astronomy and Astrophysics; October 2009, Vol. 506 Issue: 1 p95-101, 7p
Publication Year :: 2009
Abstract: Context. Be stars undergo outbursts producing a circumstellar disk from the ejected material. The beating of non-radial pulsations has been put forward as a possible mechanism of ejection.

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