Multicolour studies of β Cephei stars in the LMC

Details Multicolour studies of β Cephei stars in the LMC Multicolour studies of β Cephei stars in the LMC

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..286e&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Other

Stars: Early-Type, Techniques: Photometric, Stars: Variables: Other

Scientific paper

Preliminary results of a four-week multi-colour photometric campaign on previously identified β Cephei stars as well as newly-discovered variable stars in two respective LMC fields are presented. Besides the two targeted β Cephei stars, at least six further presumed B variables are detected. The strongest identified periods appear to lie on the longward end of the galactic β Cep instability strip, as predicted by model calculations.

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