New observational results on pulsating B stars

Details New observational results on pulsating B stars New observational results on pulsating B stars

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004coast.145...74p&link_type=abstract

Communications in Asteroseismology, vol. 145, p. 74-79

Physics

1

Scientific paper

The paper summarizes recent observational results concerning pulsating main-sequence B-type stars: Beta Cephei and SPB. In particular, recent studies of Galactic open clusters and Magellanic Clouds led to the discovery of many Beta Cephei stars. These results confirm observationally the strong dependence of the pulsation mechanism of Beta Cephei stars on metallicity, predicted by theory. New findings in the follow-up observations of SPB stars and asteroseismology of Beta Cephei stars are also described.

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