An analysis of water line profiles in star formation regions observed by the Submillimeter Wave Astronomy Satellite

Astrophysical Journal

Volumn 539, Issue 2 PART 2, 2000, Pages

  Ashby, M L N ^a   Bergin, E A ^a   Plume, R ^a   Carpenter, J M ^b   Neufeld, D A ^c   Chin, G ^d   Erickson, N R ^e   Goldsmith, P F ^f   Harwit, M ^g   Howe, J E ^e   Kleiner, S C ^a   Koch, D G ^h   Patten, B M ^a   Schieder, R ⁱ   Snell, R L ^e   Stauffer, J R ^a   Tolls, V ^a   Wang, Z ^a   Winnewisser, G ⁱ   Zhang, Y F ^a   Melnick, G J ^a   more..

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e UNIVERSITY OF MASSACHUSETTS   (United States)

^f Department of Obstetrics Gynecology   (United States)

^g NASA Ames Research Center ^*  (United States)

^h NASA AMES RESEARCH CENTER   (United States)

ⁱ UNIVERSITY OF COLOGNE   (Germany)

Author keywords

ISM: clouds; ISM: molecules; Radio lines:ISM; Stars: formation

Indexed keywords

EID: 0040145228     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/312842     Document Type: Article

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