On the origin of the recently discovered ultra-rapid pulsar
| dc.contributor.author | Radhakrishnan, V | |
| dc.contributor.author | Srinivasan, G | |
| dc.date.accessioned | 2005-12-26T09:14:36Z | |
| dc.date.available | 2005-12-26T09:14:36Z | |
| dc.date.issued | 1982-12-05 | |
| dc.description.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 X 10^-19 ss-1 for this pulsar. The gravitational radiation from this pulsar is expected to be negligible. | en |
| dc.format.extent | 272756 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Current Science, 1982, Vol. 51, p1096-1099. | en |
| dc.identifier.issn | 0011-3891 | |
| dc.identifier.uri | http://hdl.handle.net/2289/874 | |
| 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 origin of the recently discovered ultra-rapid pulsar | en |
| dc.type | Article | en |