On the implications of the radio and x-ray pulsar in the supernova  remnant MSH 15-52

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/875

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DC Field	Value	Language
dc.contributor.author	Srinivasan, G.	-
dc.contributor.author	Dwarakanath, K.S.	-
dc.contributor.author	Radhakrishnan, V.	-
dc.date.accessioned	2005-12-26T09:21:02Z	-
dc.date.available	2005-12-26T09:21:02Z	-
dc.date.issued	1982-06-20	-
dc.identifier.citation	Current Science, 1982, Vol. 51, p596-599.	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2289/875	-
dc.description.abstract	Comparison of the X-ray nebulosity surrounding the X-ray and radio pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an initial period for the pulsar ~ 70 ms. The association of the pulsar with the shell remnant confirms the validity of the ∑-t approach in determining the ages of young SNRs using historical calibrators.	en
dc.format.extent	288594 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 implications of the radio and x-ray pulsar in the supernova remnant MSH 15-52	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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