What is the nature of the central compact X-ray source in the supernova remnant RCW 103
| dc.creator | Popov, S. B. | |
| dc.date | 1998-06-26 | |
| dc.date | 1998-07-20 | |
| dc.date.accessioned | 2026-07-07T02:27:17Z | |
| dc.date.available | 2026-07-07T02:27:17Z | |
| dc.description | In this poster I discuss the nature of the compact X-ray source in the center of the supernova remnant RCW 103. Several models, based on the accretion onto a compact object such as a neutron star or a black hole (isolated or binary), are analyzed. I show that it is more likely that the central X-ray source is an accreting neutron star than an accreting black hole. I also argue that models of a disrupted binary system consisting of an old accreting neutron star and a new one observed as a 69-ms X-ray and radio pulsar are most favored. | |
| dc.description | 8 pages, no figures, to be presented as a poster at the conference "Non-accelerator particle astrophysics" 29 June - 10 July 1998, Trieste, Italy. In the replaced version a short note about earlier discussion by Torii et al. was added | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9806354 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9806354 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12628 | |
| dc.subject | Astrophysics | |
| dc.title | What is the nature of the central compact X-ray source in the supernova remnant RCW 103 | |
| dc.type | text |