General Relativistic effects of rotation on the structure and surface redshift of fast pulsars

dc.contributor.author	Datta, B
dc.contributor.author	Kapoor, R. C
dc.date.accessioned	2005-12-07T04:31:03Z
dc.date.available	2005-12-07T04:31:03Z
dc.date.issued	1984-12
dc.identifier.citation	BASI, Vol. 12, No. 4, pp. 343-349	en
dc.identifier.uri	http://hdl.handle.net/2248/634
dc.description.abstract	General relativistic effects of rotation on the structure and surface emission of the fast pulsar PSR 1937 + 214 are illustrated using a rotationally perturbed interior spherical metric. The results are found to differ markedly from those derived on the basis of simple spherical models, and are expected to be generally valid for the class of fast pulsars.	en
dc.format.extent	546521 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	General relativity	en
dc.subject	Neutron star structure	en
dc.subject	Fast Pulsars	en
dc.subject	Redshift	en
dc.title	General Relativistic effects of rotation on the structure and surface redshift of fast pulsars	en
dc.type	Article	en