A radiation driven implosion model for the enhanced luminosity of protostars near HII regions

Astronomy and Astrophysics

Volumn 467, Issue 2, 2007, Pages 657-664

  Motoyama, K ^a   Umemoto, T ^b   Shang, H ^c  

^a NATIONAL TSING HUA UNIVERSITY   (Taiwan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

Author keywords

ISM: HII regions; Methods: numerical; Stars: formation

Indexed keywords

COMPUTER SIMULATION; DENSITY (SPECIFIC GRAVITY); LUMINANCE; NUMERICAL METHODS; SOLAR RADIATION;

MOLECULAR CLOUDS; PROTOSTARS; STARS: FORMATION;

STARS;

EID: 34249341765     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20067042     Document Type: Article

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