Two-dimensional models of layered protoplanetary discs - I. The ring instability

Monthly Notices of the Royal Astronomical Society

Volumn 362, Issue 1, 2005, Pages 361-368

  Wunsch R ^a,c   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, accretion discs; Hydrodynamics; Instabilities; Solar system: formation

Indexed keywords

STABILITY;

ACCRETION: ACCRETION DISKS; AXIALLY SYMMETRIC; DEAD ZONES; HYDRODYNAMIC CODES; PROTOPLANETARY DISKS; RADIATION HYDRODYNAMICS; SOLAR SYSTEM FORMATION; SYMMETRIC MODEL; TWO DIMENSIONAL MODEL; TWO-DIMENSIONAL;

HYDRODYNAMICS;

EID: 24944566382     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09319.x     Document Type: Article

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