Blueshift and spectral features of the gravitational searchlight

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4342

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DC Field	Value	Language
dc.contributor.author	Chitre, S. M	-
dc.contributor.author	Narlikar, J. V	-
dc.contributor.author	Kapoor, R. C	-
dc.date.accessioned	2009-02-05T11:42:12Z	-
dc.date.available	2009-02-05T11:42:12Z	-
dc.date.issued	1975-10	-
dc.identifier.citation	General Relativity and Gravitation, Vol. 6, No. 5, pp. 477 - 487	en
dc.identifier.issn	1572-9532	-
dc.identifier.uri	http://hdl.handle.net/2248/4342	-
dc.description	Restricted Access	-
dc.description.abstract	It is shown that a photon emitted in the forward direction by a charged particle moving in an equatorial circular orbit centred on a highly collapsed mass M, the radius being slightly in excess of one and a half times the Schwarzschild radius, is strongly blueshifted when it arrives at a distant receiver. A ring shaped emitting region composed of such orbiting particles has a power law spectrum of the formdν/ν as seen by a distant stationary observer.	en
dc.language.iso	en	en
dc.publisher	Plenum Publishing Corporation	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00762452	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1975GReGr...6..477C	en
dc.subject	Blueshift	en
dc.subject	Gravitational searchlight	en
dc.title	Blueshift and spectral features of the gravitational searchlight	en
dc.type	Article	en
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