Gas-phase CO2, C2H2, and HCN toward Orion-KL

Astronomy and Astrophysics

Volumn 399, Issue 3, 2003, Pages 1047-1061

  Boonman, A M S ^a   Van Dishoeck, E F ^a   Lahuis, F ^a,b   Doty, S D ^c   Wright, C M ^d   Rosenthal, D ^e  

^a LEIDEN UNIVERSITY   (Netherlands)

^b SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^c DENISON UNIVERSITY   (United States)

^d UNIVERSITY OF NEW SOUTH WALES   (Australia)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

ISM: abundances; ISM: individual objects: Orion IRc2, Peak 1, Peak 2; ISM: lines and bands; ISM: molecules; Molecular processes; Stars: formation

Indexed keywords

ATMOSPHERIC CHEMISTRY; ATMOSPHERIC TEMPERATURE; CARBON DIOXIDE; EVAPORATION; GALAXIES; GAS ABSORPTION; GAS EMISSIONS; INFRARED RADIATION; INFRARED SPECTROSCOPY; MATHEMATICAL MODELS; OBSERVATORIES; SPECTROMETERS;

EXCITATION TEMPERATURES; INFRARED SPACE OBSERVATORY; SHORT WAVELENGTH SPECTROMETER;

ASTROPHYSICS;

EID: 0037373824     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021799     Document Type: Article

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