Feedback Processes in Massive Star Formation
Abstract
We present new algorithms for the efficient inclusion of radiative feedback in hydrodynamic simulations of massive star formation. Radiation pressure on dust is studied in the context of Bondi Hoyle accretion in cluster cores and photoionisation feedback incorporated in highly inhomogeneous molecular clouds
- Publication:
-
Revista Mexicana de Astronomia y Astrofisica Conference Series
- Pub Date:
- December 2004
- Bibcode:
- 2004RMxAC..22..123C
- Keywords:
-
- H II regions;
- ISM: Jets and outflows;
- Stars: Mass loss;
- Stars: Pre-main sequence