The interaction of a jet-like pulse with a wind from a stellar companion
| dc.creator | Riera, A. | |
| dc.creator | Raga, A. C. | |
| dc.creator | Alcolea, J. | |
| dc.date | 2005-03-01 | |
| dc.date.accessioned | 2026-07-07T02:17:07Z | |
| dc.date.available | 2026-07-07T02:17:07Z | |
| dc.description | We present numerical simulations of the interaction between a collimated, bipolar ``pulse'' ejected from a star and a continuous wind ejected from a stellar companion. We explore the characteristics of the predicted H$α$ intensity maps by varying selected input parameters. We find that the asymmetry (in size and strength) between the two lobes of the proto-planetary nebula OH 231.8+4.2 is reproduced in this scenario if the wind ejected by the companion star has a strong latitude dependence. | |
| dc.description | 8 pages, 7 figures, accepted for publication by RevMexAA | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0503020 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0503020 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/9054 | |
| dc.subject | Astrophysics | |
| dc.title | The interaction of a jet-like pulse with a wind from a stellar companion | |
| dc.type | text |