On the origin of the recently discovered ultra-rapid pulsar

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/874

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DC Field	Value	Language
dc.contributor.author	Radhakrishnan, V.	-
dc.contributor.author	Srinivasan, G.	-
dc.date.accessioned	2005-12-26T09:14:36Z	-
dc.date.available	2005-12-26T09:14:36Z	-
dc.date.issued	1982-12-05	-
dc.identifier.citation	Current Science, 1982, Vol. 51, p1096-1099.	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2289/874	-
dc.description.abstract	The rapid rotation rate of ~ 1.5 ms of the newly discovered pulsar PSR 1937 + 21 is attributed to spin-up in a long-lived mass transfer binary. Such a history leads to a prediction of a very low period derivative ~ 6 X 10^-19 ss-1 for this pulsar. The gravitational radiation from this pulsar is expected to be negligible.	en
dc.format.extent	272756 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.title	On the origin of the recently discovered ultra-rapid pulsar	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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