A line survey of Orion KL from 325 to 360 GHz

Astrophysical Journal, Supplement Series

Volumn 108, Issue 1, 1997, Pages 301-337

  Schilke, P ^a,b   Groesbeck, T D ^a   Blake, G A ^a   Phillips, T G ^a  

^a California Institute of Technology   (United States)

^b UNIVERSITY OF COLOGNE   (Germany)

Author keywords

ISM: abundances; ISM: individual (Orion Kleinmann Low); Line: identification; Radio lines: ISM

Indexed keywords

CARBON MONOXIDE; CARBONYL SULFIDE; HYDROCARBON; HYDROGEN CYANIDE; NITRIC OXIDE; SILICON DERIVATIVE; SULFIDE; SULFUR DIOXIDE; SULFUR OXIDE;

ARTICLE; ASTRONOMY; GAS; METHODOLOGY; MICROCLIMATE; SPECTROSCOPY;

ASTRONOMY; CARBON MONOXIDE; EXTRATERRESTRIAL ENVIRONMENT; GASES; HYDROCARBONS; HYDROGEN CYANIDE; NITRIC OXIDE; SILICON COMPOUNDS; SPECTRUM ANALYSIS; SULFIDES; SULFUR DIOXIDE; SULFUR OXIDES;

EID: 34547650114     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/312948     Document Type: Article

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