Modification of AGB wind in a binary system
| dc.creator | Frankowski, Adam | |
| dc.creator | Tylenda, Romuald | |
| dc.date | 2000-02-25 | |
| dc.date.accessioned | 2026-07-07T01:52:31Z | |
| dc.date.available | 2026-07-07T01:52:31Z | |
| dc.description | We explore one of plausible causes of asymmetry in the wind of an AGB star - the presence of a binary companion. We have developed a simple method for estimating the intrinsic non-sphericity of the outflow in that case. Assuming the Roche model, local stellar parameters (T_eff, g) are calculated, and then a formula for the local mass loss rate is applied. As a by-product a relation between the ratio of stellar radius to the Roche lobe radius and the overall wind enhancement is obtained. | |
| dc.description | 4 pages, 5 figures. To appear in ``Asymmetrical Planetary Nebulae II: from Origins to Microstructures,'' ASP Conference Series, J.H. Kastner, N. Soker, & S.A. Rappaport, eds | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0002486 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0002486 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/647 | |
| dc.subject | Astrophysics | |
| dc.title | Modification of AGB wind in a binary system | |
| dc.type | text |