Three-dimensional molecular line transfer: A simulated star-forming region

Monthly Notices of the Royal Astronomical Society

Volumn 407, Issue 2, 2010, Pages 986-1002

  Rundle, David ^a   Harries, Tim J ^a   Acreman, David M ^a   Bate, Matthew R ^a  

^a UNIVERSITY OF EXETER   (United Kingdom)

Author keywords

ISM: kinematics and dynamics; ISM: molecules; Methods: numerical; Radiative transfer; Stars: formation

Indexed keywords

CODES (SYMBOLS); DENSITY OF GASES; GASES; HYDRODYNAMICS; MESH GENERATION; NUMERICAL METHODS; STARS; VELOCITY;

ADAPTIVE MESHES; ISM: KINEMATICS AND DYNAMICS; ISM:MOLECULES; LEVEL POPULATIONS; LOCAL THERMODYNAMIC EQUILIBRIUM; METHOD: NUMERICAL; MOLECULAR LINES; NONLOCAL; SMOOTHED PARTICLE HYDRODYNAMICS; STARS FORMATION;

RADIATIVE TRANSFER;

EID: 77956405634     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16982.x     Document Type: Article

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