The eclipsing binary SV Cam shows photometric features that suggest its membership to the RS CVn group. The existing light curves (covering the period 1947 - 1986) have been analyzed in order to isolate the contribution of the wave-like distortion; all the observations support the presence of an activity cycle, with a duration of about 10 years.
Rapid time variability in the short-period RS CVn-type binary SV Camelopardalis
BUSSO, Maurizio Maria
Investigation
;
1987
Abstract
The eclipsing binary SV Cam shows photometric features that suggest its membership to the RS CVn group. The existing light curves (covering the period 1947 - 1986) have been analyzed in order to isolate the contribution of the wave-like distortion; all the observations support the presence of an activity cycle, with a duration of about 10 years.File in questo prodotto:
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