Has the Crab Pulsar magnetic field grown after its birth?
| dc.contributor.author | Bhattacharya, D | |
| dc.contributor.author | Shukre, C S | |
| dc.date.accessioned | 2006-01-04T05:43:51Z | |
| dc.date.available | 2006-01-04T05:43:51Z | |
| dc.date.issued | 1985 | |
| dc.description.abstract | The evolution of rotation period and spindown age of a pulsar whose surface magnetic field undergoes a phase of growth were investigated. Application of these results to the Crab pulsar strongly indicates that its parameters cannot be accounted for by the field growth theories. | en |
| dc.format.extent | 490069 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Journal of Astrophysics and Astronomy, 1985, Vol. 6, p233-237. | en |
| dc.identifier.issn | 0250-6335 | |
| dc.identifier.uri | http://hdl.handle.net/2289/1078 | |
| dc.language.iso | en | en |
| dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
| dc.rights | Indian Academy of Sciences, Bangalore, India. | en |
| dc.subject | Pulsars | en |
| dc.subject | Magnetic field | en |
| dc.subject | Evolution - Pulsars | en |
| dc.title | Has the Crab Pulsar magnetic field grown after its birth? | en |
| dc.type | Article | en |