Three-dimensional models of embedded high-mass stars: Effects of a clumpy circumstellar medium

Astrophysical Journal

Volumn 636, Issue 1 I, 2006, Pages 362-380

  Indebetouw, R ^a   Whitney, B A ^b   Johnson, K E ^a   Wood, K ^c  

^a UNIVERSITY OF VIRGINIA   (United States)

^b Cassini Imaging Central Laboratory for Operations   (United States)

^c UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Circumstellar matter; Dust, extinction; Radiative transfer; Stars: Formation; Stars: Pre main sequence

Indexed keywords

EID: 33645670918     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/497886     Document Type: Article

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