Distortion wave characteristics and starspot modelling in the RS CVn eclipsing binary SV Camelopardalis

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1420

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DC Field	Value	Language
dc.contributor.author	Sarma, C. V. S. R	-
dc.contributor.author	Vivekananda, P	-
dc.contributor.author	Sarma, M. B. K	-
dc.date.accessioned	2007-03-14T06:41:13Z	-
dc.date.available	2007-03-14T06:41:13Z	-
dc.date.issued	1990	-
dc.identifier.citation	BASI, Vol. 18, pp. 253-259	en
dc.identifier.uri	http://hdl.handle.net/2248/1420	-
dc.description.abstract	Four migrating groups of wave minima are identified in the light curves of SV Cam of which two show direct motion with period 3.02 and 1.6 yr while the other two display retrograde motion with periods 3.04 and 0.6 yr. Based on the methodology of Budding, the four groups of spots are modeled to fit the distortion wave modulations. It is noticed that two of the spot groups, direct I and retrograde I, have preferred quadrature positions while the other two, direct II and retrograde II, are found to be at random positions. The sizes of starspots generally tended to diminish with time	en
dc.format.extent	190194 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Starspots	en
dc.title	Distortion wave characteristics and starspot modelling in the RS CVn eclipsing binary SV Camelopardalis	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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