The circumstellar environments of high-mass protostellar objects: I. Submillimetre continuum emission

Astronomy and Astrophysics

Volumn 417, Issue 1, 2004, Pages 115-133

  Williams, S J ^a   Fuller, G A ^a   Sridharan, T K ^b  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

ISM: clouds; ISM: dust, extinction; Stars: circumstellar matter; Stars: formation

Indexed keywords

APPROXIMATION THEORY; CLOUDS; DUST; MORPHOLOGY; OPTICAL RESOLVING POWER; PROBABILITY;

EXTINCTION; ISM: CLOUDS; ISM: DUST; STARS: CIRCUMSTELLAR MATTER; STARS: FORMATION;

ASTROPHYSICS;

EID: 1842425842     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031733     Document Type: Article

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