Numerical requirements for simulations of self-gravitating and non-self-gravitating discs

Monthly Notices of the Royal Astronomical Society

Volumn 373, Issue 3, 2006, Pages 1039-1073

  Nelson, Andrew F ^a,b,c  

^a UNIVERSITY OF EDINBURGH   (United Kingdom)

^b UKAFF   (United States)

^c LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

Hydrodynamics; Methods: numerical; Planetary systems: protoplanetary discs; Solar system: formation

Indexed keywords

GRAVITATION; NUMERICAL METHODS; PLANETS; SOLAR SYSTEM; STABILITY; STARS;

AVERAGE NUMBERS; CONDITION; GRID-BASED SIMULATION; HYDRODYNAMIC SIMULATION; METHOD: NUMERICAL; NEUTRAL STABILITY; PARTICLE SIMULATIONS; PLANETARY SYSTEMS:PROTOPLANETARY DISKS; SOLAR SYSTEM FORMATION; VERTICAL STRUCTURES;

HYDRODYNAMICS;

EID: 33845343576     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11119.x     Document Type: Article

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