Clumps and shocks in the outer winds of hot stars
Abstract
We present a moving periodic box technique to study the outer-wind evolution of instability-generated structure in hot-star winds. This has considerable computational and conceptual advantages
- Publication:
-
A Massive Star Odyssey: From Main Sequence to Supernova
- Pub Date:
- 2003
- Bibcode:
- 2003IAUS..212..226R