Probing the formation of intermediate- To high-mass stars in protoclusters II. Comparison between millimeter interferometric observations of NGC 2264-C and SPH simulations of a collapsing clump

Astronomy and Astrophysics

Volumn 464, Issue 3, 2007, Pages 983-994

  Peretto, N ^a,c   Hennebelle, P ^b   Andre P ^a  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b ECOLE NORMALE SUPÉRIEURE   (France)

^c UNIVERSITY OF MANCHESTER   (United Kingdom)

Author keywords

Hydrodynamics; ISM; Ism: clouds; Kinematics and dynamics; Stars: circumstellar matter; Stars: formation; Stars: kinematics

Indexed keywords

CLOUDS; COMPUTER SIMULATION; GRAVITATIONAL EFFECTS; HYDRODYNAMICS; INTERFEROMETRY; KINEMATICS;

CIRCUMSTELLAR MATTER; MILLIMETER INTERFEROMETRIC OBSERVATIONS; PROTOCLUSTERS; STAR FORMATION;

STARS;

EID: 33947730186     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065653     Document Type: Article

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