Pulsations, chemical composition and multiplicity in main-sequence A- and F-type stars

Details Pulsations, chemical composition and multiplicity in main-sequence A- and F-type stars Pulsations, chemical composition and multiplicity in main-sequence A- and F-type stars

2009-01-20

arxiv.org/abs/0901.3162v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Contribution to the Proceedings of the Wroclaw HELAS Workshop, 2008, to appear in Communications in Asterseismology, 157

Scientific paper

The region in the HR-diagram where the main sequence intersects the classical instability strip hosts A- and F-type stars exhibiting a rich variety of physical phenomena, such as pulsations on various time scales and chemical peculiarities. We aim to investigate the occurrence of these phenomena among suspected binary systems in this region of the HR-diagram and their mutual interactions.

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