Two-dimensional models of layered protoplanetary discs - II. The effect of a residual viscosity in the dead zone

Monthly Notices of the Royal Astronomical Society

Volumn 367, Issue 2, 2006, Pages 773-780

  Wunsch R ^a,c   Gawryszczak, A ^a   Klahr, H ^b   Rozyczka M ^a  

^a NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c ASTRONOMICAL INSTITUTE   (Czech Republic)

Author keywords

Accretion discs; Hydrodynamics; Instabilities; Solar system:formation

Indexed keywords

ACCRETION DISCS; ACCRETION RATE; ANALYTICAL DESCRIPTION; AXISYMMETRIC MODELING; DEAD ZONES; OSCILLATORY INSTABILITY; PROTOPLANETARY DISKS; RADIATIVE TRANSFER EFFECTS; SOLAR SYSTEM FORMATION; TWO DIMENSIONAL MODEL;

VISCOSITY;

EID: 33645081721     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09986.x     Document Type: Article

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