Temperature and brightness distributions in the components of close binary system

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