Some arguments in support of the association of PSR B1706-44 with the supernova remnant G343.1-2.3
| dc.creator | Bock, Douglas C. -J. | |
| dc.creator | Gvaramadze, V. V. | |
| dc.date | 2001-11-22 | |
| dc.date.accessioned | 2026-07-07T02:01:28Z | |
| dc.date.available | 2026-07-07T02:01:28Z | |
| dc.description | We present some arguments in support of the association of the pulsar PSR B1706-44 with the supernova remnant G343.1-2.3, based on the idea that these objects could be the result of a supernova explosion within a mushroom-like cavity (created by the supernova progenitor wind breaking out of the parent molecular cloud). We suggest that in addition to the known bright "half" of G343.1-2.3 there should exist a more extended and weaker component, such that the actual shape of G343.1-2.3 is similar to that of the well-known SNR VRO 42.05.01. We have found such a component in archival radio data. | |
| dc.description | (4 pages) To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M. Gaensler | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0111430 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0111430 | |
| dc.identifier | ASP Conf.Ser. 271 (2002) 49 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3757 | |
| dc.subject | Astrophysics | |
| dc.title | Some arguments in support of the association of PSR B1706-44 with the supernova remnant G343.1-2.3 | |
| dc.type | text |