Smoothed particle hydrodynamics simulations of expanding H II regions I. Numerical method and applications

Astronomy and Astrophysics

Volumn 497, Issue 2, 2009, Pages 649-659

  Bisbas, T G ^a   Wunsch R ^a   Whitworth, A P ^a   Hubber, D A ^a,b  

^a CARDIFF UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF OSLO   (Norway)

Author keywords

ISM: HII regions; Methods: numerical; Radiative transfer

Indexed keywords

ANGULAR RESOLUTIONS; COMPUTATIONAL COSTS; DENSE GAS; DYNAMICAL EFFECTS; H II REGIONS; INTERSTELLAR MEDIUMS; IONIZATION EQUILIBRIUMS; ISM: HII REGIONS; METHODS: NUMERICAL; NEGATIVE FEEDBACKS; POSITIVE FEEDBACKS; SELF-PROPAGATING; SMOOTHED PARTICLE HYDRODYNAMICS; SPH SIMULATIONS; STAR FORMATIONS; TEMPERATURE INCREASE; THREE ORDERS OF MAGNITUDES;

ADAPTIVE ALGORITHMS; FEEDBACK; FLUID DYNAMICS; IONIZATION OF GASES; IONIZING RADIATION; RADIATION EFFECTS; RADIATION SHIELDING; RADIATIVE TRANSFER; RADIOACTIVITY;

NUMERICAL METHODS;

EID: 65349142691     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811522     Document Type: Article

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