Linking pre- and proto-stellar objects in the intermediate-/high-mass star forming region IRAS 05345+3157

Astronomy and Astrophysics

Volumn 499, Issue 1, 2009, Pages 233-247

  Fontani, F ^a,b   Zhang, Q ^c   Caselli, P ^d   Bourke, T L ^c  

^a UNIVERSITY OF GENEVA   (Switzerland)

^b UNIVERSITÉ DE GENÈVE   (Switzerland)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY OF LEEDS   (United Kingdom)

Author keywords

ISM: molecules; Stars: formation

Indexed keywords

COLD CONDENSATION; COLUMN DENSITY; CONTINUUM SOURCE; DEUTERIUM FRACTIONATION; DRIVING SOURCE; HIGH ANGULAR RESOLUTIONS; HIGH-ANGULAR RESOLUTION; HIGH-MASS STARS; INITIAL CONDITIONS; ISM: MOLECULES; LOW-MASS; MOLECULAR LINES; PRIMARY BEAMS; PROTOSTAR; PROTOSTARS; STAR-FORMATION PROCESS; STARS: FORMATION; VELOCITY GRADIENTS;

DEUTERIUM; KINEMATICS; STARS;

CONDENSATION;

EID: 66349125968     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911617     Document Type: Article

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