The importance of non-LTE models for the interpretation of observations of interstellar NO

Astronomy and Astrophysics

Volumn 493, Issue 2, 2009, Pages 557-563

  Lique, F ^a,b,e   Van Der Tak, F F S ^c   Klos J ^b   Bulthuis, J ^d   Alexander, M H ^b  

^a CNRS   (France)

^b Bldg 142   (United States)

^c SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^d VU UNIVERSITY AMSTERDAM   (Netherlands)

^e UNIVERSITÉ DU HAVRE   (France)

Author keywords

ISM: molecules; Molecular data; Radiative transfer

Indexed keywords

ASTROPHYSICS; GEOPHYSICS; HELIUM; MOLECULES; RADIATION; RADIATIVE TRANSFER;

AMBIENT TEMPERATURES; COLLISIONAL RATES; COLUMN DENSITIES; CRITICAL DENSITIES; FAR-INFRARED; HYPERFINE LEVELS; ISM: MOLECULES; LINE EMISSIONS; LINE RATIOS; MOLECULAR DATA; NO EMISSIONS; RADIATIVE TRANSFER CODES; RATE COEFFICIENTS; ROTATIONAL EXCITATIONS; ROTATIONAL LINES; SUB-MILLIMETER WAVELENGTHS; VELOCITY GRADIENTS;

KNOWLEDGE BASED SYSTEMS;

EID: 59049099050     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810453     Document Type: Article

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