Three-dimensional simulations of globule and pillar formation around HII regions: Turbulence and shock curvature

Astronomy and Astrophysics

Volumn 546, Issue , 2012, Pages

  Tremblin, P ^a   Audit, E ^a,b   Minier, V ^a   Schmidt, W ^c   Schneider, N ^a  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b LABORATOIRE DES SCIENCES DU CLIMAT ET DE L ENVIRONNEMENT   (France)

^c UNIVERSITY OF GÖTTINGEN   (Germany)

Author keywords

HII regions; ISM: structure; Methods: numerical; Stars: formation; Turbulence

Indexed keywords

COLD GAS; DENSE SHELLS; DENSITY STRUCTURES; DOUBLE PEAK STRUCTURE; H II REGIONS; IONIZED MEDIUM; ISM: STRUCTURE; LOCAL CURVATURE; MASSIVE STARS; METHODS: NUMERICALS; MOLECULAR CLOUDS; MOLECULAR GAS; NONEQUILIBRIUM MODEL; PILLAR FORMATION; STARS: FORMATION; THERMAL PROCESS; THREE DIMENSIONAL SIMULATIONS; THREE-DIMENSIONAL (3D) NUMERICAL SIMULATIONS; TURBULENT MEDIUM;

GASES; MACH NUMBER; NUMERICAL METHODS; PROBABILITY DENSITY FUNCTION; SHELLS (STRUCTURES); STARS; THREE DIMENSIONAL; THREE DIMENSIONAL COMPUTER GRAPHICS; TURBULENCE;

IONIZATION OF GASES;

EID: 84866936875     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219224     Document Type: Article

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