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2008CoAst.152..160H - Com. in Asteroseismology, 152, 160 (2008/January-0)
$β$∼Cephei and slowly pulsating b stars as targets for BRITE- constellation.
HANDLER G.
Abstract (from CDS):
We discuss the potential of BRITE-Constellation for asteroseismology of main sequence B-type pulsators. We briefly review previous asteroseismic work on these oscillators and point out the importance of these stars astrophysics in general. We find that BRITE-Constellation is ideally suited for studying B-type pulsators, and we identify several interesting regions in the sky that may be observed.
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Simbad objects: 4
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