Gamma rays from millisecond pulsars.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/744

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DC Field	Value	Language
dc.contributor.author	Bhattacharya, D.	-
dc.contributor.author	Srinivasan, G.	-
dc.date.accessioned	2005-12-16T09:25:59Z	-
dc.date.available	2005-12-16T09:25:59Z	-
dc.date.issued	1991-02-11	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1991, Vol. 12, p17-25.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/744	-
dc.description.abstract	The contribution of millisecond pulsars to the diffuse gamma-ray background of the Galaxy is estimated, and it is shown that a significant fraction of the Galactic background may originate from them. A small number of the unidentified COS-B point sources may, in fact, be millisecond pulsars. It is argued that several hundred millisecond pulsars may be detectable as point sources by the GRO satellite.	en
dc.format.extent	789791 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	Pulsars	en
dc.subject	Millisecond-gamma-ray emission	en
dc.subject	Diffuse gamma- ray background	en
dc.title	Gamma rays from millisecond pulsars.	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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