Hydrodynamical interaction between an accretion flow and a stellar wind
| dc.creator | Mendoza, S. | |
| dc.creator | Canto, J. | |
| dc.creator | Raga, A. | |
| dc.date | 2004-01-21 | |
| dc.date | 2004-04-22 | |
| dc.date.accessioned | 2026-07-25T12:11:27Z | |
| dc.description | Molecular clouds in the interstellar medium suffer gravitational instabilities that lead to the formation of one or multiple stars. A recently formed star inside a cold cloud communicates its gravitational force to the surrounding environment and soon an accretion flow falling into the star develops. After their formation, all stars soon eject a wind of gas that interacts with the external accretion flow. This interaction produces a shock wave that evolves with time. The work presented in this article formulates a simple prescription for the evolution of this interaction. With the aid of this model we construct a few radio continuum maps of the source. | |
| dc.description | 42 pages, 13 figures. Minor changes done to the first draft. Accepted for publication in RevMexAA | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0401426 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0401426 | |
| dc.identifier | Rev.Mex.Astron.Astrofis. 40 (2004) 147-165 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/8147 | |
| dc.subject | Astrophysics | |
| dc.title | Hydrodynamical interaction between an accretion flow and a stellar wind | |
| dc.type | text |