The role of the energy equation in the fragmentation of protostellar discs during stellar encounters

Monthly Notices of the Royal Astronomical Society

Volumn 374, Issue 2, 2007, Pages 590-598

  Lodato, G ^a   Meru, F ^a   Clarke, C J ^a   Rice, W K M ^b  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF EDINBURGH   (United Kingdom)

Author keywords

Accretion, accretion discs; Gravitation; Instabilities; Planetary systems: formation; Stars: formation; Stars: low mass, brown dwarfs

Indexed keywords

HEATING; HYDRODYNAMICS; STARS;

ACCRETION: ACCRETION DISKS; ENERGY EQUATION; HIGH RESOLUTION; HYDRODYNAMIC SIMULATION; PLANETARY SYSTEMS:FORMATION; PROTOSTELLAR DISKS; SMOOTHED PARTICLE HYDRODYNAMICS; STARS FORMATION; STARS: LOW-MASS BROWN DWARFS; STELLARS;

GRAVITATION;

EID: 33846136406     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11211.x     Document Type: Article

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