β Cephei and Slowly Pulsating B stars as targets for BRITE- Constellation

Details β Cephei and Slowly Pulsating B stars as targets for BRITE- Constellation β Cephei and Slowly Pulsating B stars as targets for BRITE- Constellation

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.152..160h&link_type=abstract

Communications in Asteroseismology, Vol.152, p. 160-165

Astronomy and Astrophysics

Astrophysics

Scientific paper

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 for 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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