Temperature and brightness distribution in the components of binary systems

dc.contributor.author	Barman, S. K
dc.date.accessioned	2007-04-13T09:54:18Z
dc.date.available	2007-04-13T09:54:18Z
dc.date.issued	1993-03
dc.identifier.citation	BASI, Vol. 21, No.1, pp 27-32	en
dc.identifier.uri	http://hdl.handle.net/2248/1474
dc.description.abstract	From the theoretical model of a binary system for gravity darkening (Barman 1991), the temperature and brightness distributions along the surface of the components have been calculated using the third and fourth orders of the ratio (r/R) in the tidal potentials created by the secondary components, where r is radial distance and R the distance between the centers of gravities of the binary stars. Results of both distributions have been presented in seven figures. On analyzing the results, it has been suggested that if the expansion technique be used to calculate the combined potentials and related matters e.g. the temperature and brightness distributions of a binary system, one should at least consider the fourth order of the ratio (r/R).	en
dc.format.extent	362987 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Binary stars	en
dc.subject	Gravity darkening	en
dc.title	Temperature and brightness distribution in the components of binary systems	en
dc.type	Article	en