Ionization feedback in star formation simulations: The role of diffuse fields

Monthly Notices of the Royal Astronomical Society

Volumn 413, Issue 1, 2011, Pages 401-410

  Ercolano, Barbara ^a,b,c   Gritschneder, Matthias ^d  

^a UNIVERSITY OF EXETER   (United Kingdom)

^b UNIVERSITY OF MUNICH   (Germany)

^c EXCELLENCE CLUSTER UNIVERSE   (Germany)

^d PEKING UNIVERSITY   (China)

Author keywords

ISM: structure; Radiative transfer; Stars: formation; Turbulence

Indexed keywords

CODES (SYMBOLS); HYDRODYNAMICS; IONIZATION OF GASES; STARS; TEMPERATURE DISTRIBUTION; TURBULENCE;

DIFFUSE FIELDS; FORMATION SIMULATION; GAS TEMPERATURE DISTRIBUTIONS; INTERSTELLAR MEDIAS; INTERSTELLAR MEDIUM: STRUCTURE; MEDIA STRUCTURE; ON THE SPOTS; PROPERTY; SMOOTH PARTICLE HYDRODYNAMICS; STARS FORMATION;

RADIATIVE TRANSFER;

EID: 84856214494     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18144.x     Document Type: Article

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