The stellar mass spectrum from non-isothermal gravoturbulent fragmentation

Astronomy and Astrophysics

Volumn 435, Issue 2, 2005, Pages 611-623

  Jappsen, A K ^a   Klessen, R S ^a   Larson, R B ^b   Li, Y ^c,d   Low, M M Mac ^c,d  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b YALE UNIVERSITY   (United States)

^c DIVISION OF INVERTEBRATE ZOOLOGY   (United States)

^d Och Spine at New York Presbyterian Hospitals   (United States)

Author keywords

Equation of state; Hydrodynamics; ISM: clouds; Methods: numerical; Stars: formation; Turbulence

Indexed keywords

CLOUDS; COMPUTER SIMULATION; EQUATIONS OF STATE; GRAVITATION; HYDRODYNAMICS; ISOTHERMS; MOLECULAR PHYSICS; THERMODYNAMICS; TURBULENCE;

ISM: CLOUDS; METHODS: NUMERICAL; STAR-FORMING GAS; STARS: FORMATION;

ASTRONOMY;

EID: 18744410666     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042178     Document Type: Article

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