Effects of rotation and tidal distortions on the equilibrium structure and periods of oscillations of stars in binary systems

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1428

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DC Field	Value	Language
dc.contributor.author	Mohan, C	-
dc.contributor.author	Saxena, R. M	-
dc.date.accessioned	2007-03-14T08:37:44Z	-
dc.date.available	2007-03-14T08:37:44Z	-
dc.date.issued	1990	-
dc.identifier.citation	BASI, Vol. 18, pp. 315-328	en
dc.identifier.uri	http://hdl.handle.net/2248/1428	-
dc.description.abstract	Methods for computing the equilibrium structures and periods of barotropic modes of oscillations of stars which are the primary components of binary systems are presented. The methods utilize the averaging technique of Kippenhahn and Thomas (1970) and the concepts of Roche equipotentials to incorporate rotational and tidal effects. The use of the methods in obtaining the equilibrium structures and eigenfrequencies of barotropic modes of oscillations of certain polytropic models of stars (assumed to be the primary components of synchronous as well as nonsynchronous binary systems) is also illustrated	en
dc.format.extent	357409 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	-
dc.subject	Binary stars	en
dc.subject	Oscillations	en
dc.title	Effects of rotation and tidal distortions on the equilibrium structure and periods of oscillations of stars in binary systems	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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