Radiatively driven winds: shaping bipolar LBV nebulae
Abstract
Massive stars which are fast rotators can give rise to asymmetric winds. These winds may result in the formation of aspherical wind-blown nebulae. In this work the theory of radiatively-driven winds from massive stars is used to model the formation of bipolar nebulae around LBV stars.
- Publication:
-
A Massive Star Odyssey: From Main Sequence to Supernova
- Pub Date:
- 2003
- Bibcode:
- 2003IAUS..212..172D