Temperature and brightness distributions in the components of close binary system

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1442

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DC Field	Value	Language
dc.contributor.author	Barman, S. K	-
dc.date.accessioned	2007-03-14T10:11:34Z	-
dc.date.available	2007-03-14T10:11:34Z	-
dc.date.issued	1991	-
dc.identifier.citation	BASI, Vol. 19, No. 1&2, pp. 59-64	en
dc.identifier.uri	http://hdl.handle.net/2248/1442	-
dc.description.abstract	A theoretical model of close binary system for the gravity-darkening due to tidally and nonuniformly rotating Roche components has been formulated using the fourth order of r/R where r is the radial distance and R is the distance between the centers of the binary stars. This model provides expressions to calculate the temperature and brightness distributions along the surface of the components	en
dc.format.extent	289306 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Binary stars	en
dc.title	Temperature and brightness distributions in the components of close binary system	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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