Srinivasan, G. ; Bhattacharya, D. (1984) On the nature of the Supernova Remnant 0540-69.3 in the Large Magellanic Cloud Current Science, 53 (10). pp. 513-516. ISSN 0011-3891
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Official URL: http://www.ias.ac.in/j_archive/currsci/53/10/513-5...
Abstract
The implications of the recently discovered X-ray pulsar within the SNR 0540-69.3 in the Large Magellanic Cloud is investigated. It is suggested that the SNR is a shell-plerion combination.
| Item Type: | Article |
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| Source: | Copyright of this article belongs to Current Science Association. |
| ID Code: | 55562 |
| Deposited On: | 18 Aug 2011 11:31 |
| Last Modified: | 18 May 2016 07:47 |
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