Srinivasan, G. ; Dwarakanath, K. S. ; Radhakrishnan, V. (1982) On the implications of the radio and X-ray pulsar in the Supernova Remnant MSH 15-52 Current Science, 51 (12). pp. 596-599. ISSN 0011-3891
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Official URL: http://www.ias.ac.in/j_archive/currsci/51/12/596-5...
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.
| Item Type: | Article |
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| Source: | Copyright of this article belongs to Current Science Association. |
| ID Code: | 55558 |
| Deposited On: | 18 Aug 2011 11:31 |
| Last Modified: | 18 May 2016 07:47 |
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