On The Variability of 27 Cygni
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Nancy Remage Evans
Space Physics Laboratory, Institue for Space and Terrestrial Studies, York University
4700 Keele Street, North York, Ontario, Canada M5S 1A1
John R. Percy
Department of Astronomy, University of Toronto, Toronto, Ontario, Canada M5S 1A1
Received: 11 April 1989
Abstract
We report on the analysis of three seasons of photoelectric photometry of 27 Cygni (KOIV) and
one season of radial velocities. The star shows marginal (but probably real) variability in both
light and velocity, on a time scale of weeks. further study of the star does not seem to be
warranted, but it should not be used as a comparison star for differential photometry of other
variable stars.
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