The thermodynamics of molecular cloud fragmentation star formation under non-Milky Way conditions

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Hocuk, S ^a   Spaans, M ^a  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

Author keywords

Dust, extinction; Equation of state; Hydrodynamics; ISM: clouds; Stars: formation; Turbulence

Indexed keywords

3D SIMULATIONS; ADAPTIVE MESH REFINEMENT CODES; AMBIENT CONDITIONS; COOLING FUNCTION; DENSE CORE; DUST , EXTINCTION; DWARF GALAXIES; EQUATION OF STATE; ISM : CLOUDS; MASS FUNCTIONS; METALLICITIES; MILKY WAYS; MOLECULAR CLOUDS; NUMBER DENSITY; ROTATIONAL ENERGY; STAR FORMATIONS; STARBURSTS; STARS: FORMATION; THERMAL BALANCE; THERMODYNAMIC EFFECT;

ASTROPHYSICS; COSMIC RAYS; DUST; EQUATIONS OF STATE; FLUID DYNAMICS; GALAXIES; HEATING; HYDRODYNAMICS; STARS; THERMODYNAMICS; THREE DIMENSIONAL COMPUTER GRAPHICS; TURBULENCE;

CLOUDS;

EID: 79952843835     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912236     Document Type: Article

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