A new algorithm for radiative feedback and its application to the formation of massive stars

Monthly Notices of the Royal Astronomical Society

Volumn 338, Issue 4, 2003, Pages 962-972

  Edgar, Richard ^a   Clarke, Cathie ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

Hydrodynamics; Methods: Numerical; Radiative transfer; Stars: Early type stars: Formation

Indexed keywords

DUST; MIXTURES; NUMERICAL METHODS; RADIATIVE TRANSFER; STARS;

EARLY-TYPE - STARS; FEEDBACK APPLICATIONS; FREQUENCY-DEPENDENT; ITS APPLICATIONS; MASSIVE STARS; METHOD: NUMERICAL; SIMPLIFIED METHOD; STAR: EARLY-TYPE STAR: FORMATION; STARS FORMATION; STARS:EARLY TYPE;

HYDRODYNAMICS;

EID: 0141955935     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06139.x     Document Type: Article

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