The formation of protestellar disks. III. The influence of gravitationally induced angular momentum transport on disk structure and appearance

Astrophysical Journal

Volumn 525, Issue 1 PART 1, 1999, Pages 330-342

  Yorke, Harold W ^a,b,c   Bodenheimer, Peter ^c  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b Astronomisches Institut   (Germany)

^c University of California Santa Cruz   (United States)

Author keywords

Hydrodynamics; ISM: clouds radiative transfer; stars: formation

Indexed keywords

EID: 0033227548     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/307867     Document Type: Article

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