Dwarf cepheid AD CMi -- revisited

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1476

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DC Field	Value	Language
dc.contributor.author	Kilambi, G. C	-
dc.contributor.author	Rahman, A	-
dc.date.accessioned	2007-04-13T11:14:56Z	-
dc.date.available	2007-04-13T11:14:56Z	-
dc.date.issued	1993-03	-
dc.identifier.citation	BASI, Vol. 21, No. 1, pp 47-61	en
dc.identifier.uri	http://hdl.handle.net/2248/1476	-
dc.description.abstract	An analysis of UBVR light variations of AD Canis Minoris (CMi) is presented. The mean effective temperature derived from the intrinsic (B - V) index is estimated to be 7400 K +/- 100 K whereas that of the (V - R) index value is 8425 K +/- 120 K. The mean variation of temperature from the (B - V) index over a pulsation cycle is almost twice that of the estimated (V - R) index value. The estimated mass, radius and effective gravity values suggest that AD CMi is a normal population-I pulsating star and a member of the delta-Scuti group.	en
dc.format.extent	1054588 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Variable star	en
dc.subject	Photometry	en
dc.title	Dwarf cepheid AD CMi -- revisited	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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