Long-Term Timing of 374 Pulsars
| dc.creator | Hobbs, G. | |
| dc.creator | Lyne, A. | |
| dc.creator | Kramer, M. | |
| dc.date | 2003-10-03 | |
| dc.date.accessioned | 2026-07-07T02:09:58Z | |
| dc.date.available | 2026-07-07T02:09:58Z | |
| dc.description | We have analysed the arrival times for 374 pulsars that have been observed for more than six years using the 76-m Lovell telescope at Jodrell Bank Observatory. Here we present a qualitative analysis of structures seen in the timing residuals. | |
| dc.description | To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310093 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310093 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6634 | |
| dc.subject | Astrophysics | |
| dc.title | Long-Term Timing of 374 Pulsars | |
| dc.type | text |