A radiation-driven disc wind model for massive young stellar objects

Monthly Notices of the Royal Astronomical Society

Volumn 296, Issue 1, 1998, Pages

  Drew, Janet E ^a   Proga, Daniel ^a   Stone, James M ^b  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b Bldg 142   (United States)

Author keywords

Accretion, accretion discs; Circumstellar matter; Hydrodynamics; Methods: numerical; Stars: mass loss; Stars: pre main sequence

Indexed keywords

FLUID DYNAMICS; NUMERICAL METHODS;

ACCRETION: ACCRETION DISKS; BE STARS; CIRCUMSTELLAR MATTERS; DRIVEN DISCS; METHOD: NUMERICAL; STARS: MASS-LOSS; STARS: PRE-MAIN SEQUENCE; WIND MODELLING; YOUNG STELLAR OBJECTS;

STARS;

EID: 0041170714     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01438.x     Document Type: Article

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