Short-Period Photometric Variability of the Be-Star 28-CYGNI

Details Short-Period Photometric Variability of the Be-Star 28-CYGNI Short-Period Photometric Variability of the Be-Star 28-CYGNI

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pasp...93..460s&link_type=abstract

Publications of the Astronomical Society of the Pacific, Vol. 93, P. 460, 1981

Astronomy and Astrophysics

Astronomy

9

Scientific paper

Observations in the UBV system are reported for the Be star 28 Cyg. The short-period variability initially reported in 1976 has apparently increased in amplitude and in July 1978 a 0d.7 periodicity was detected during four days of observations. It is speculated that this quasi-periodic behavior may be related to the axial rotation of the star.

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