| dc.creator | Curé, M. | |
| dc.creator | Rial, D. F. | |
| dc.creator | Cidale, Lydia Sonia | |
| dc.date | 2005-07-03 | |
| dc.date | 2019-10-16T15:28:16Z | |
| dc.identifier | http://sedici.unlp.edu.ar/handle/10915/83382 | |
| dc.identifier | issn:0004-6361 | |
| dc.description | The effects of rapid rotation and bi-stability upon the density contrast between the equatorial and polar directions of a B[e] supergiant are re-investigated. Based on a new slow solution for different high rotational radiation-driven winds and the fact that bi-stability allows a change in the line-force parameters (α, k, and δ), the equatorial densities are about 102-104 times higher than the polar ones. These values are in qualitative agreement with the observations. | |
| dc.description | Facultad de Ciencias Astronómicas y Geofísicas | |
| dc.format | application/pdf | |
| dc.format | 929-933 | |
| dc.language | en | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/4.0/ | |
| dc.rights | Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) | |
| dc.subject | Ciencias Astronómicas | |
| dc.subject | Stars: early-type | |
| dc.subject | Stars: mass-loss | |
| dc.subject | Stars: rotation | |
| dc.subject | Stars: winds, outflows | |
| dc.title | Outflowing disk formation in B supergiants due to rotation and bi-stability in radiation driven winds | |
| dc.type | Articulo | |
| dc.type | Articulo | |
