White dwarf origin of SN 1987a

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1089

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DC Field	Value	Language
dc.contributor.author	Srinivasan, G.	-
dc.date.accessioned	2006-01-04T11:07:13Z	-
dc.date.available	2006-01-04T11:07:13Z	-
dc.date.issued	1987-03-20	-
dc.identifier.citation	Current Science, 1987, Vol. 56, p245 -249.	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2289/1089	-
dc.description.abstract	We argue that the recently discovered supernova in the Large Magellanic Cloud represents the transition of a white dwarf to a neutron star in a binary system. The rapid rise to maximum light, the very subluminous nature and reports of the detection of neutrinos from the event are fully consistent with the proposed model.	en
dc.format.extent	346491 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	White dwarf origin of SN 1987a	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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