Radhakrishnan, V. ; Srinivasan, G. (1982) On the origin of the recently discovered ultra-rapid pulsar Current Science, 51 (23). pp. 1096-1099. ISSN 0011-3891
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Official URL: http://www.ias.ac.in/j_archive/currsci/51/23/1096-...
Abstract
The rapid rotation rate of ~ 1.5 ms of the newly discovered pulsar PSR 1937 + 21 is attributed to spin-up in a long-lived mass transfer binary. Such a history leads to a prediction of a very low period derivative ~ 6 × 10−19 ss−1 for this pulsar. The gravitational radiation from this pulsar is expected to be negligible.
| Item Type: | Article |
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| Source: | Copyright of this article belongs to Current Science Association. |
| ID Code: | 55563 |
| Deposited On: | 18 Aug 2011 11:31 |
| Last Modified: | 18 May 2016 07:47 |
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