"High-field" pulsars torqued by accretion disk?
| dc.creator | Yue, Y. L. | |
| dc.creator | Zhu, W. W. | |
| dc.creator | Xu, R. X. | |
| dc.date | 2006-11-02 | |
| dc.date.accessioned | 2026-07-07T07:30:37Z | |
| dc.date.available | 2026-07-07T07:30:37Z | |
| dc.description | The nature of AXPs/SGRs (anomalous X-ray pulsars/soft $γ$-ray repeaters) and high field radio pulsars is still unclear even in the magnetar and/or accretion models. The detection of radio emission from AXP XTE J1810$-$197 and the discovery of a debris disk around AXP 4U 0142+61 might shed light on the problem. We propose that AXPs/SGRs could be pulsars that have magnetic field $B\lesssim 10^{13} \mathrm{G}$ as normal pulsars, but in accretion environments. We investigate these issues under the accretion model and find that two of the AXPs/SGRs might be low mass quark stars if all AXPs and SGRs are likely grouped together. | |
| dc.description | 6 pages, 1 figures, submitted to "Advances in Space Research" (Proceedings of COSPAR 2006) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611041 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611041 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/118467 | |
| dc.subject | Astrophysics | |
| dc.title | "High-field" pulsars torqued by accretion disk? | |
| dc.type | text |