The NH2D/NH3 ratio toward pre-protostellar cores around the UC H(ii) region in IRAS 20293+3952

Astronomy and Astrophysics

Volumn 517, Issue 7, 2010, Pages

  Busquet, G ^a   Palau, A ^b   Estalella, R ^a   Girart, J M ^b   Sanchez Monge A ^a   Viti, S ^c   Ho, P T P ^d,e   Zhang, Q ^d  

^a UNIVERSITY OF BARCELONA   (Spain)

^b UNIVERSITAT AUTÒNOMA DE BARCELONA   (Spain)

^c UNIVERSITY COLLEGE LONDON   (United Kingdom)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

Author keywords

ISM: clouds; ISM: individual objects: IRAS 20293+3952; ISM: molecules; Stars: formation

Indexed keywords

DEUTERIUM; STARS; ULTRAVIOLET RADIATION;

CLUSTER ENVIRONMENTS; DEUTERIUM FRACTIONATION; DUST EMISSION; HIGH ANGULAR RESOLUTIONS; ISM : CLOUDS; ISM: MOLECULES; LOW-MASS STARS; UV RADIATION; YOUNG STELLAR OBJECTS;

CLOUDS;

EID: 77955453352     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014866     Document Type: Article

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