On the origin of H2CO abundance enhancements in low-mass protostars

Astronomy and Astrophysics

Volumn 418, Issue 1, 2004, Pages 185-202

  Schoier F L ^a,b   Jorgensen J K ^a   Van Dishoeck, E F ^a   Blake, G A ^c  

^a LEIDEN UNIVERSITY   (Netherlands)

^b STOCKHOLM OBSERVATORY   (Sweden)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Astrochemistry; ISM: abundances; Stars: circumstellar matter; Stars: formation; Stars: individual: IRAS 16293 2422, L1448 C

Indexed keywords

CARBON MONOXIDE; CONTINUUM MECHANICS; EVAPORATION; HEATING; HYDROGEN INORGANIC COMPOUNDS; ICE; INTERFEROMETERS; MATHEMATICAL MODELS; MORPHOLOGY; PARTICULATE EMISSIONS; ROTATION; SILICON COMPOUNDS;

ASTROCHEMISTRY; ISM:ABUNDANCES; STARS:CIRCUMSTELLAR MATTER; STARS:FORMATION; STARS:INDIVIDUAL:IRAS 16293-2422; STARS:INDIVIDUAL:L1448-C;

ASTROPHYSICS;

EID: 2342502604     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035769     Document Type: Article

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