The effect of a finite mass reservoir on the collapse of spherical isothermal clouds and the evolution of protostellar accretion

Monthly Notices of the Royal Astronomical Society

Volumn 360, Issue 2, 2005, Pages 675-684

  Vorobyov, E I ^a,b   Basu, Shantanu ^a  

^a UNIVERSITY OF WESTERN ONTARIO   (Canada)

^b SOUTHERN FEDERAL UNIVERSITY   (Russian Federation)

Author keywords

Hydrodynamics; ISM: Clouds; Stars: Formation

Indexed keywords

DENSITY OF GASES; HYDRODYNAMICS; ISOTHERMS; LUMINANCE;

ACCRETION RATE; CLASS I; DENSITY PROFILE; FINITE MASS; ISM : CLOUDS; PROTOSTARS; RAREFACTION WAVES; SELF-SIMILAR; STARS FORMATION; STELLARS;

STARS;

EID: 20744459729     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09062.x     Document Type: Article

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