Highly deuterated pre-stellar cores in a high-mass star formation region

Astronomy and Astrophysics

Volumn 477, Issue 3, 2008, Pages

  Fontani, F ^a   Caselli, P ^b,c   Bourke, T L ^d   Cesaroni, R ^b   Brand, J ^a  

^a OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^c UNIVERSITY OF LEEDS   (United Kingdom)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

ISM: individual: IRAS 05345+3157; ISM: molecules; Radio lines: ISM; Stars: formation

Indexed keywords

DEUTERIUM; HIGH FREQUENCY TELECOMMUNICATION LINES; INTERFEROMETERS; MORPHOLOGY; OPTICAL RESOLVING POWER; PARAMETER ESTIMATION;

DEUTERATED GAS; DEUTERIUM FRACTIONATION; PRE STELLAR CORES;

STARS;

EID: 38049130405     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078973     Document Type: Article

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