On the association between pulsars and supernova remnants

Radhakrishnan, V.; Srinivasan, G.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2427

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DC Field	Value	Language
dc.contributor.author	Radhakrishnan, V.	-
dc.contributor.author	Srinivasan, G.	-
dc.date.accessioned	2007-05-25T08:45:34Z	-
dc.date.available	2007-05-25T08:45:34Z	-
dc.date.issued	1983	-
dc.identifier.citation	IAU Symposium, 1983, Vol.101, p487-494	en
dc.identifier.uri	http://hdl.handle.net/2289/2427	-
dc.description	Open Access. Supernova remnants and their X-ray emission; Proceedings of the Symposium, Venice, Italy, August 30-September 2, 1982 (A84-43078 21-90). Dordrecht, D. Reidel Publishing Co., 1983	en
dc.description.abstract	Available data on associations between pulsars and supernova remnants (SNR) are surveyed for possible conclusions that may be drawn. Pulsars have been detected in the Crab and Vela SNR. The pulsar in Vela is at the periphery of the nebula at the edge of the shell, whereas the shell energy may be derived from other neutron stars in Vela. Calculations of the pulsar birthrate are consistent with the current discovery rate and birthrate of SNRs. It is possible that all SN produce pulsars, some which never reach a detectable, active stage. Finally, the Crab Nebula is regarded as an atypical situation.	en
dc.format.extent	865798 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Reidel	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1983IAUS..101..487R	en
dc.rights	1983 Reidel	en
dc.subject	Pulsars	en
dc.subject	Supernova Remnants	en
dc.subject	Crab nebula	en
dc.subject	Neutron stars	en
dc.title	On the association between pulsars and supernova remnants	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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