A three-position spectral line survey of Sagittarius B2 between 218 and 263 GHz. I. The observational data

Astrophysical Journal, Supplement Series

Volumn 117, Issue 2, 1998, Pages 427-529

  Nummelin, A ^a   Bergman, P ^a   Hjalmarson, A ^a   Friberg, P ^b   Irvine, W M ^c   Millar, T J ^d   Ohishi, M ^e   Saito, S ^f  

^a CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^b UNIVERSITY OF HAWAII   (United States)

^c UNIVERSITY OF MASSACHUSETTS   (United States)

^d UNIVERSITY OF MANCHESTER   (United Kingdom)

^e NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^f INSTITUTE FOR MOLECULAR SCIENCE   (Japan)

Author keywords

ISM: individual (Sagittarius B2); ISM: molecules; Line: identification; Surveys

Indexed keywords

EID: 0042278827     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/313126     Document Type: Article

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