Modeling gas-phase H2O between 5 μm and 540 μm toward massive protostars

Astronomy and Astrophysics

Volumn 406, Issue 3, 2003, Pages 937-955

  Boonman, A M S ^a   Doty, S D ^b   Dishoeck, E F ^a   Bergin, E A ^c   Melnick, G J ^c   Wright, C M ^a   Stark, R ^d  

^a LEIDEN UNIVERSITY   (Netherlands)

^b DENISON UNIVERSITY   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Infrared: ISM; ISM: abundances; ISM: lines and bands; ISM: molecules; Molecular processes

Indexed keywords

ASTRONOMICAL SATELLITES; COMPUTER SIMULATION; EVAPORATION; GASES; ICE; INFRARED RADIATION; LIGHT ABSORPTION; MOLECULES; SPACE TELESCOPES; SPECTROMETERS;

ABUNDANCES; INFRARED SPACE OBSERVATORY; PROTOSTARS; RADIATIVE TRANSFER MODEL;

GALAXIES;

EID: 0041696870     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030765     Document Type: Article

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