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