Investigation of X-ray transient CI Cam as an unique star with the B[e]phenomenon

Details Investigation of X-ray transient CI Cam as an unique star with the B[e]phenomenon Investigation of X-ray transient CI Cam as an unique star with the B[e]phenomenon

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..602b&link_type=abstract

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

Astronomy and Astrophysics

Astronomy

Binaries: General, Novae, Cataclysmic Variables, Stars: Oscillations (Including Pulsations), Circumstellar Matter

Scientific paper

Double mode pulsations of the B4 component in the system of CI Cam were detected. The photometric 19.4 day orbital period of CI Cam was confirmed with the plates of the Sonneberg collection for a long period of time before the unique 1998 outburst. The amplitude of the periodic component of 0.08 mag before the outburst was larger than that of 0.03 mag after the outburst.

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