The pulsations of the B5IVe star HD 181231observed with CoRoT and ground-based spectroscopy ***

Authors :: Neiner, C.
Gutiérrez-Soto, J.
Baudin, F.
de Batz, B.
Frémat, Y.
Huat, A. L.
Floquet, M.
Hubert, A.-M.
Leroy, B.
Diago, P. D.
Poretti, E.
Carrier, F.
Rainer, M.
Catala, C.
Thizy, O.
Buil, C.
Ribeiro, J.
Andrade, L.
Emilio, M.
Espinosa Lara, F.
Fabregat, J.
Janot-Pacheco, E.
Martayan, C.
Semaan, T.
Suso, J.
Baglin, A.
Michel, E.
Samadi, R.
Neiner, C.
Gutiérrez-Soto, J.
Baudin, F.
de Batz, B.
Frémat, Y.
Huat, A. L.
Floquet, M.
Hubert, A.-M.
Leroy, B.
Diago, P. D.
Poretti, E.
Carrier, F.
Rainer, M.
Catala, C.
Thizy, O.
Buil, C.
Ribeiro, J.
Andrade, L.
Emilio, M.
Espinosa Lara, F.
Fabregat, J.
Janot-Pacheco, E.
Martayan, C.
Semaan, T.
Suso, J.
Baglin, A.
Michel, E.
Samadi, R.
Source :: Astronomy and Astrophysics; October 2009, Vol. 506 Issue: 1 p143-151, 9p
Publication Year :: 2009
Abstract: Context. HD 181231is a B5IVe star, which has been observed with the CoRoT satellite during ~5 consecutive months and simultaneously from the ground in spectroscopy and spectropolarimetry.

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