Feedback Processes in Massive Star Formation

Details Feedback Processes in Massive Star Formation Feedback Processes in Massive Star Formation

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..22..123c&link_type=abstract

Gravitational Collapse: From Massive Stars to Planets. / First Astrophysics meeting of the Observatorio Astronomico Nacional. /

Astronomy and Astrophysics

Astrophysics

H Ii Regions, Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

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

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