Recent photometry of CG Cygni

Details Recent photometry of CG Cygni Recent photometry of CG Cygni

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93..210n&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 93, Jan. 1987, p. 210-213. Research supported by Pitzer College.

Astronomy and Astrophysics

Astronomy

11

Binary Stars, Light Curve, Stellar Spectrophotometry, Ultraviolet Astronomy

Scientific paper

The authors present three seasons (1981, 1982, 1983) of new photometry of the short-period RS CVn-like system CG Cygni. The system's period continues to steadily increase. The steady brightening of the system appears to have ended. The distortion wave varies erratically, and may not be migrating in a uniform manner. A brief episode of excess light, seen near secondary eclipse, is probably due to a hot gas stream.

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