Young close isolated compact objects
| dc.creator | Popov, S. B. | |
| dc.creator | Prokhorov, M. E. | |
| dc.creator | Colpi, M. | |
| dc.creator | Treves, A. | |
| dc.creator | Turolla, R. | |
| dc.date | 2002-01-03 | |
| dc.date.accessioned | 2026-07-07T02:02:07Z | |
| dc.date.available | 2026-07-07T02:02:07Z | |
| dc.description | We suggest that the seven radio-quiet isolated neutron stars observed with ROSAT are young cooling objects associated to recent near-by supernova explosions which formed runaway stars and the Local Bubble, affecting the topology of the interstellar medium in the vicinity of the Sun (within a few hundred parsecs). In the aftermath of these explosions, a few black holes might have been formed, according to the local initial mass function. We thus discuss the possibility of determining approximate positions of close-by isolated black holes using data on runaway stars and simple calculations of binary evolution and disruption. | |
| dc.description | 4 pages, no figures, to appear in proceedings of the conference ICGA-V in Gravitation & Cosmology (2002) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0201030 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0201030 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3980 | |
| dc.subject | Astrophysics | |
| dc.title | Young close isolated compact objects | |
| dc.type | text |