Distribution of the luminosity of accreting isolated compact objects
| dc.creator | Popov, S. B. | |
| dc.creator | Prokhorov, M. E. | |
| dc.date | 1997-05-29 | |
| dc.date | 1997-06-16 | |
| dc.date.accessioned | 2026-07-07T09:02:10Z | |
| dc.date.available | 2026-07-07T09:02:10Z | |
| dc.description | We present here the computer model of the distribution of the luminosity, produced by old isolated neutron stars and black holes accreting from the interstellar medium in the Galaxy in R-Z plane. We show, that the luminosity distributions have a torus-like structure, with the maximum at $\approx 5-6 kpc$. | |
| dc.description | 4 pages, 6 PostScript figures. Uses l-aa style. To be presented as a poster at the conference "Neutron stars - 97", St. Petersburg, June 9-11, 1997. In the replaced version fig. 3 and 5 are changed | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9705236 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9705236 | |
| dc.identifier | A&A V. 331, p.535 (1998) | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/148534 | |
| dc.subject | Astrophysics | |
| dc.title | Distribution of the luminosity of accreting isolated compact objects | |
| dc.type | text |