Beta Cephei pulsation and the helium-strong stars

Details Beta Cephei pulsation and the helium-strong stars Beta Cephei pulsation and the helium-strong stars

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1461m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Nov. 1988, p. 1461-1464. Research supported by NSE

Astronomy and Astrophysics

Astronomy

1

B Stars, Cepheid Variables, Peculiar Stars, Stellar Atmospheres, Stellar Composition, Astronomical Photometry, Helium, Periodic Variations, Stellar Envelopes

Scientific paper

The authors identify six He-strong stars which may be good candidates in
searches for β Cephei pulsation based on their location in a plot
of β vs. [u - b]. The significance of detection of pulsational
variability among the He-peculiar stars in the study of excitation
mechanisms for β Cephei stars is discussed.

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