On the relationship between pulsars and supernova remnants

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4115

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DC Field	Value	Language
dc.contributor.author	Kochhar, R. K	-
dc.date.accessioned	2008-12-18T14:21:36Z	-
dc.date.available	2008-12-18T14:21:36Z	-
dc.date.issued	1981-03	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 2, pp. 87 - 93	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2248/4115	-
dc.description.abstract	We propose that single stars in the mass range 4–6·5M ⊙, that explode as Supernovae of Type I, are totally disrupted by the explosion and form shell-type remnants. More massive single stars which explode as Supernovae of Type II also give rise to shell-type remnants, but in this case a neutron star or a black hole is left behind. The first supernova explosion in a close binary also gives rise to a shell-type supernova remnant. The Crab-like filled-centre supernova remnants are formed by the second supernova explosion in a close binary. The hybrid supernova remnants, consisting of a filled centre surrounded by a shell, are formed if there is an active neutron star inside the shell.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1981JApA....2...87K	en
dc.relation.uri	http://dx.doi.org/10.1007/BF02714245	en
dc.subject	Pulsars	en
dc.subject	Supernovae	en
dc.subject	Supernova remnants	en
dc.title	On the relationship between pulsars and supernova remnants	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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