Depletion and low gas temperature in the L183 (=L134N) prestellar core: The N2H+-N2D+ tool

Astronomy and Astrophysics

Volumn 467, Issue 1, 2007, Pages 179-186

  Pagani, L ^a   Bacmann, A ^b   Cabrit, S ^a   Vastel, C ^c  

^a OBSERVATOIRE DE PARIS   (France)

^b UNIVERSITÉ DE BORDEAUX   (France)

^c IRAP   (France)

Author keywords

ISM: abundances; ISM: individual objects: L183; ISM: molecules; ISM: structure; Line: formation; Radiative transfer

Indexed keywords

ASTROPHYSICS; ATMOSPHERIC COMPOSITION; MONTE CARLO METHODS; RADIATIVE TRANSFER;

ANTENNA BEAM; HYPERFINE TRANSITIONS; PRE-STELLAR CORES (PSC);

STARS;

EID: 34249280615     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066670     Document Type: Article

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