Numerical simulations of continuum-driven winds of super-Eddington stars

Monthly Notices of the Royal Astronomical Society

Volumn 389, Issue 3, 2008, Pages 1353-1359

  Van Marle, A J ^a   Owocki, S P ^a   Shaviv, N J ^b  

^a UNIVERSITY OF DELAWARE   (United States)

^b HEBREW UNIVERSITY OF JERUSALEM   (Israel)

Author keywords

Hydrodynamics; Methods: numerical; Stars: mass loss; Stars: winds, outflows

Indexed keywords

NUMERICAL METHODS; NUMERICAL MODELS; PHOTONS; STARS;

ANALYTICAL SCALING; CONDITION; METHOD: NUMERICAL; OPTICAL THICKNESS; PARAMETER STUDIES; PROPERTY; STARS: MASS-LOSS; STARS: WINDS OUTFLOWS; STELLAR ATMOSPHERES; WIND MODELLING;

WIND;

EID: 51349106589     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13648.x     Document Type: Article

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