The Formation of Protostellar Disks. III. The Influence of Gravitationally Induced Angular Momentum Transport on Disk Structure and Appearance
Author(s) -
H. W. Yorke,
Peter Bodenheimer
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/307867
Subject(s) - physics , protostar , angular momentum , astrophysics , accretion (finance) , radiative transfer , specific relative angular momentum , hydrostatic equilibrium , radius , thick disk , gravitational collapse , total angular momentum quantum number , astronomy , stars , star formation , classical mechanics , angular momentum coupling , computer security , quantum mechanics , galaxy , computer science , halo
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