Propiedades de los Vientos de Estrellas Supergigantes B
Abstract
The winds of B-type Supergiant stars are not completely consistent with the solutions of the classical line-driven winds theory. In this work we study the properties of those winds, by modeling Hα line profiles with the code FASTWIND and fitting them to a set of high resolution observations. We also find the main parameters for these objects. FULL TEXT IN SPANISH
- Publication:
-
Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
- Pub Date:
- 2012
- Bibcode:
- 2012BAAA...55...95H