Bibcode
Liu, Y. Y.; Jiang, S. Y.; Michel, E.; Hernandez, M. M.; Chevreton, M.; Auvergne, M.; Mangeney, A.; Belmonte, J. A.; Goupil, M. J.; Baglin, A.; Roca-Cortés, T.; Vidal, I.
Referencia bibliográfica
Astronomy and Astrophysics Supplement, v.120, p.179-186
Fecha de publicación:
11
1996
Número de citas
10
Número de citas referidas
6
Descripción
This paper reports on the fifth STEPHI multi-site photometric campaign
in 1993 devoted to the δ Scuti star BDS 1269A (VW Ari). The
observation yielded a data set of 150.7 hours. Our analysis has resulted
in 7 identified frequencies. These frequencies exhibit three
couple-frequency character, and also fit the previous investigations
quite well. An attempt to identify the pulsation modes is made, but no
equidistant evidence can be detected, and a second-order effect for
rotational splitting has to be considered to explain the complicated
nature of BDS 1269A.