Chemical modeling of L183 (L134N): An estimate of the ortho/para H 2 ratio

Astronomy and Astrophysics

Volumn 494, Issue 2, 2009, Pages 623-636

  Pagani, L ^a   Vastel, C ^b   Hugo, E ^c   Kokoouline, V ^d   Greene, C H ^e   Bacmann, A ^f   Bayet, E ^g   Ceccarelli, C ^f   Peng, R ^h   Schlemmer, S ^c  

^a OBSERVATOIRE DE PARIS   (France)

^b IRAP   (France)

^c UNIVERSITY OF COLOGNE   (Germany)

^d UNIVERSITY OF CENTRAL FLORIDA   (United States)

^e UNIVERSITY OF COLORADO   (United States)

^f UNIV GRENOBLE ALPES   (France)

^g UNIVERSITY COLLEGE LONDON   (United Kingdom)

^h Caltech Submillimeter Observatory   (United States)

Author keywords

Astrochemisty; ISM: abundances; ISM: clouds; ISM: individual objects: L183; ISM: structure; Molecular processes

Indexed keywords

AMPLIFICATION; CLOUDS; DEUTERIUM; DISSOCIATION; HYDROGEN; POSITIVE IONS;

ASTROCHEMISTY; ISM: ABUNDANCES; ISM: CLOUDS; ISM: INDIVIDUAL OBJECTS: L183; ISM: STRUCTURE; MOLECULAR PROCESSES;

REACTION RATES;

EID: 59649123196     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810587     Document Type: Article

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