Testing the locality of transport in self-gravitating accretion discs

Monthly Notices of the Royal Astronomical Society

Volumn 351, Issue 2, 2004, Pages 630-642

  Lodato, G ^a   Rice, W K M ^b  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Accretion, accretion discs; Galaxies: active; Gravitation; Instabilities; Stars: formation

Indexed keywords

ASPECT RATIO; ENERGY DISSIPATION; GALAXIES; HYDRODYNAMICS; STRESS TENSOR;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; CONDITION; GALAXIES ACTIVE; GRAVITATIONAL INSTABILITY; HYDRODYNAMIC SIMULATION; PARAMETRIZATIONS; SIMPLE++; STARS FORMATION; THREE-DIMENSIONAL SMOOTHED PARTICLE HYDRODYNAMICS;

GRAVITATION;

EID: 3042853567     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07811.x     Document Type: Article

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