Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3703

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DC Field	Value	Language
dc.contributor.author	Datta, B	-
dc.contributor.author	Kapoor, R. C	-
dc.date.accessioned	2008-09-17T11:45:41Z	-
dc.date.available	2008-09-17T11:45:41Z	-
dc.date.issued	1988-08	-
dc.identifier.citation	Astrophysical Journal, Vol. 331, No. 2, Part 1, pp. 784 - 793	en
dc.identifier.issn	0004-637X	-
dc.identifier.uri	http://hdl.handle.net/2248/3703	-
dc.description.abstract	Results are presented of a study of frequency shifts in radiation from the surface of rapidly rotating neutron stars and rotation-induced spectral line broadening as a function of their mass. It is found that, despite large rotation rates, the gravitational effects dominate over the Doppler contribution to the frequency shifts over the allowed mass range of a stable rotating neutron star. Astrophysical implications of effect of large rotation on spectral line characteristics are also discussed.	en
dc.language.iso	en	en
dc.publisher	The American Astronomical Society	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1988ApJ...331..784D	en
dc.subject	Gravitational Effects	en
dc.subject	Neutron Stars	en
dc.subject	Spectral Line Width	en
dc.subject	Stellar Radiation	en
dc.subject	Stellar Rotation	en
dc.subject	Doppler Effect	en
dc.subject	Emission Spectra	en
dc.subject	Gamma Ray Bursts	en
dc.subject	Stellar Mass	en
dc.title	Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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