The present day of asteroseismology of β Cephei stars: observations

Computer Science – Databases

Scientific paper

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Scientific paper

Several successful campaigns on bright β Cephei-type pulsators were completed during the recent years yielding detections of many modes at a sub-millimag level. On the other hand, searches for β Cephei-type stars in massive photometric databases resulted in a multiplication of the number of known members of this group. These discoveries now allow much better statistical investigations of β Cephei stars as a group and a good selection of interesting targets for case studies for asteroseismology. We summarize the up-to-date achievements of asteroseismology of β Cephei stars and present the results of the searches for these stars in the OGLE, ASAS and MACHO databases.

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