Pulsations, chemical composition and multiplicity in main-sequence A- and F-type stars
Solar and Stellar Astrophysics
2009-01-22 v1
Abstract
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.
Keywords
Cite
@article{arxiv.0901.3162,
title = {Pulsations, chemical composition and multiplicity in main-sequence A- and F-type stars},
author = {S. Hekker and Y. Frémat and P. Lampens and P. De Cat},
journal= {arXiv preprint arXiv:0901.3162},
year = {2009}
}
Comments
Contribution to the Proceedings of the Wroclaw HELAS Workshop, 2008, to appear in Communications in Asterseismology, 157