Observation of Beta-Cephei Candidates in the Jewel-Box

Details Observation of Beta-Cephei Candidates in the Jewel-Box Observation of Beta-Cephei Candidates in the Jewel-Box

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.264..165k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 264, NO. 1/SEP1, P. 165, 1993

Astronomy and Astrophysics

Astronomy

8

Binaries: Eclipsing - Stars: Early-Type - Stars: Oscillations - Cepheids - Open Clusters And Associations: Individual: Ngc 4755

Scientific paper

Photometry of early B stars in the open cluster NGC 4755 confirms the previous classification of one star as a β Cephei variable. Two other β Cephei variables are found. Both primary and secondary eclipses of a binary system with a period of 1.96 d are observed. It is speculated that the β Cephei stars are pulsating in the fundamental radial or lowest order gravity modes.

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