Why do starless cores appear more flattened than protostellar cores?

Monthly Notices of the Royal Astronomical Society

Volumn 330, Issue 4, 2002, Pages 769-771

  Goodwin, S P ^a   Ward Thompson, D ^a   Whitworth, A P ^a  

^a CARDIFF UNIVERSITY   (United Kingdom)

Author keywords

Formation; Stars

Indexed keywords

GALAXIES;

AXIAL RATIO; BEST FIT; ELLIPTICAL GALAXIES; FORMATION; INTRINSIC SHAPE; MOLECULAR CORE; MOLECULAR LINES; PROJECTED SHAPES; PROTOSTARS; THREE-DIMENSIONAL SHAPE;

STARS;

EID: 0012702569     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05166.x     Document Type: Article

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