Glitch observations in slow pulsars
| dc.creator | Janssen, G. H. | |
| dc.creator | Stappers, B. W. | |
| dc.date | 2007-01-09 | |
| dc.date.accessioned | 2026-07-07T07:39:16Z | |
| dc.date.available | 2026-07-07T07:39:16Z | |
| dc.description | We have analyzed 5.5 years of timing observations of 7 ``slowly'' rotating radio pulsars, made with the Westerbork Synthesis Radio Telescope. We present improved timing solutions and 30, mostly small new glitches. The most interesting results are: 1) The detection of glitches one to two orders of magnitude smaller than ever seen before in slow radio pulsars. 2) Resolving timing-noise looking structures in the residuals of PSR B1951+32 by using a set of small glitches. 3) The detections of three new glitches in PSR J1814-1744, a high-magnetic field pulsar. In these proceedings we present the most interesting results of our study. For a full coverage, we refer the reader to Janssen & Stappers (2006). | |
| dc.description | Proceedings of the 363. WE-Heraeus Seminar on: Neutron Stars and Pulsars (Posters and contributed talks) Physikzentrum Bad Honnef, Germany, May.14-19, 2006, eds. W.Becker, H.H.Huang, MPE Report 291, pp.80-83 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701222 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701222 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/121384 | |
| dc.subject | Astrophysics | |
| dc.title | Glitch observations in slow pulsars | |
| dc.type | text |