Accretion Flows Around Black Holes
| dc.creator | Narayan, Ramesh | |
| dc.date | 1995-08-07 | |
| dc.date.accessioned | 2026-07-07T02:19:58Z | |
| dc.date.available | 2026-07-07T02:19:58Z | |
| dc.description | Most accreting black holes emit a substantial fraction of their luminosity in hard X-rays/soft $γ$-rays of up to $\sim{\rm few}\times100$ keV. The observations suggest that the radiating gas is very hot, $T>10^9$ K, and optically thin. Theoretical attempts to explain the observations are reviewed and unresolved issues are highlighted. | |
| dc.description | 20 pages, 3 figures included, compressed uuencoded Postscript, Review talk at the conference on "Some Unsolved Problems in Astrophysics," Princeton, April 27-29, 1995. To appear in the Proceedings to be published by Princeton Univ. Press (editors, J. N. Bahcall & J. P. Ostriker) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9508031 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9508031 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10077 | |
| dc.subject | Astrophysics | |
| dc.title | Accretion Flows Around Black Holes | |
| dc.type | text |