White dwarf origin of SN 1987a
| 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.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.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.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 |