Dynamics of line-driven disk winds
| dc.creator | Proga, D. | |
| dc.date | 2001-09-06 | |
| dc.date.accessioned | 2026-07-07T01:59:52Z | |
| dc.date.available | 2026-07-07T01:59:52Z | |
| dc.description | I review the main results from recent 2-D, time-dependent hydrodynamic models of radiation-driven winds from accretion disks in AGN. I also discuss the physical conditions needed for a disk wind to be shielded from the strong X-rays and to be accelerated to hypersonic velocities. I conclude with a few remarks on winds in hot stars, low mass young stellar objects, cataclysmic variables, low mass X-ray binaries, and galactic black holes and future work. | |
| dc.description | LaTeX, 6 pages, to be published in "Mass Outflow in Active Galactic Nuclei: New Perspectives" eds. D.M.Crenshaw, S.B.Kraemer and I.M.George, ASP Conf. Proc | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0109092 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0109092 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3284 | |
| dc.subject | Astrophysics | |
| dc.title | Dynamics of line-driven disk winds | |
| dc.type | text |