New aspects in the theory of magnetic winds from massive hot stars
| dc.creator | Seemann, Henning | |
| dc.date | 1998-04-16 | |
| dc.date.accessioned | 2026-07-07T02:26:36Z | |
| dc.date.available | 2026-07-07T02:26:36Z | |
| dc.description | This thesis discusses the influence of magnetic fields on the instability of line-driven winds in O-stars and Wolf-Rayet stars. This combination is an important concept to understand the strong, observed winds from Wolf-Rayet stars. In the second part of the thesis a model is derived which describes the wind outside the equatorial plane. This model allows to use the simple approach of an ordinary differential equation instead of a 2-dim. partial differential equation. | |
| dc.description | PhD thesis accepted by the university of Bonn. 79 pages with 31 Postscript figures using LaTeX2e with rotating,epsfig, amssymb&amsbsy styles | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9804152 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9804152 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12341 | |
| dc.subject | Astrophysics | |
| dc.title | New aspects in the theory of magnetic winds from massive hot stars | |
| dc.type | text |