SCOPUS 정보 검색 플랫폼

Volumn 754, Issue 1, 2012, Pages

Radiation-hydrodynamic simulations of the formation of orion-like star clusters. II. the initial mass function from winds, turbulence, and radiation

(3) Krumholz, Mark R a Klein, Richard I b,c McKee, Christopher F c

a UNIVERSITY OF CALIFORNIA (United States)

b LAWRENCE LIVERMORE NATIONAL LABORATORY (United States)

c UNIVERSITY OF CALIFORNIA (United States)

Author keywords

ISM: clouds; radiative transfer; stars: formation; stars: luminosity function, mass function; turbulence

Indexed keywords

EID: 84863706802 PISSN: 0004637X EISSN: 15384357 Source Type: Journal
DOI: 10.1088/0004-637X/754/1/71 Document Type: Article

Times cited : (263)

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