Elongated beams, interpulses and the new millisecond pulsar
| dc.contributor.author | Narayan, R | |
| dc.contributor.author | Radhakrishnan, V | |
| dc.date.accessioned | 2006-01-03T04:32:16Z | |
| dc.date.available | 2006-01-03T04:32:16Z | |
| dc.date.issued | 1983-01-20 | |
| dc.description.abstract | The prominent interpulse of the new millisecond pulsar is consistent with very short period pulsars having fan-like beams, as suggested earlier by an independent study. It is shown that all the available data on interpulse statistics support this picture, and also indicate that pulsars with perpendicular rotation and magnetic axes are absent at long periods. | en |
| dc.format.extent | 256252 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Current Science, 1983, Vol. 52, p46-49. | en |
| dc.identifier.issn | 0011-3891 | |
| dc.identifier.uri | http://hdl.handle.net/2289/1052 | |
| 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 | Elongated beams, interpulses and the new millisecond pulsar | en |
| dc.type | Article | en |