Modeling water emission from low-mass protostellar envelopes

Astronomy and Astrophysics

Volumn 487, Issue 3, 2008, Pages 975-991

  Van Kempen, T A ^a   Doty, S D ^b   Van Dishoeck, E F ^a,c   Hogerheijde, M R ^a   Jorgensen J K ^d  

^a LEIDEN UNIVERSITY   (Netherlands)

^b DENISON UNIVERSITY   (United States)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d UNIVERSITY OF BONN   (Germany)

Author keywords

Circumstellar matter; ISM: molecules; Stars: formation; Stars: pre main sequence; Submillimeter

Indexed keywords

ASTROPHYSICS; OBSERVATORIES; SPACECRAFT OBSERVATORIES; WATER PIPING SYSTEMS; WATER SUPPLY;

CIRCUMSTELLAR MATERIALS; CIRCUMSTELLAR MATTER; DENSITY PROFILES; HERSCHEL SPACE OBSERVATORY; ISM: MOLECULES; LOW-MASS; LOW-MASS STAR FORMATION; PROTOSTARS; SPHERICAL SYMMETRY; STARS: FORMATION; STARS: PRE-MAIN SEQUENCE; SUBMILLIMETER; TEMPERATURE PROFILING; WATER LINE;

WATER VAPOR;

EID: 49749106631     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809426     Document Type: Article

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