The Association of PSR B1757-24 and the SNR G5.4-1.2
| dc.creator | Gvaramadze, V. V. | |
| dc.date | 2003-10-14 | |
| dc.date.accessioned | 2026-07-07T02:10:24Z | |
| dc.date.available | 2026-07-07T02:10:24Z | |
| dc.description | The association of PSR B1757-24 and the supernova remnant (SNR) G5.4-1.2 was recently questioned by Thorsett et al. (2002) on the basis of proper motion measurements of the pulsar and the "incorrect" orientation of the vector of pulsar transverse velocity [inferred from the orientation of the cometary-shaped pulsar wind nebula (PWN)]. We showed, however, that the association could be real if both objects are the remnants of an off-centred cavity supernova (SN) explosion. | |
| dc.description | 4 pages, 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/0310380 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310380 | |
| dc.identifier | IAU Symp. 218 (2004) 77-80 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6730 | |
| dc.subject | Astrophysics | |
| dc.title | The Association of PSR B1757-24 and the SNR G5.4-1.2 | |
| dc.type | text |