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2009CoAst.159...35T - Com. in Asteroseismology, 159, 35 (2009/March-0)
Asteroseismology of b stars.
THOUL A.
Abstract (from CDS):
Numerous B stars on the main sequence are found to be variable. These stars have a relatively simple structure, and yet they present some very interesting challenges. It is important to understand these stars before we can expect to be able to understand stars which have a more complicated internal structure.
Abstract Copyright: ∼
Journal keyword(s):
Simbad objects: 5
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