Resolution requirements for simulating gravitational fragmentation using SPH

Astronomy and Astrophysics

Volumn 450, Issue 3, 2006, Pages 881-886

  Hubber, D A ^a   Goodwin, S P ^a   Whitworth, A P ^a  

^a CARDIFF UNIVERSITY   (United Kingdom)

Author keywords

Hydrodynamics; Instabilities; Methods: numerical; Stars: formation

Indexed keywords

COMPUTER SIMULATION; CRYSTALLINE MATERIALS; DENSITY (SPECIFIC GRAVITY); HYDRODYNAMICS; ISOTHERMS; NUMERICAL METHODS; OPTICAL RESOLVING POWER; PERTURBATION TECHNIQUES; PLANETS;

GRAVITATIONAL FRAGMENTATION; INSTABILITIES; SPH; STARS: FORMATION;

GRAVITATIONAL EFFECTS;

EID: 33646402046     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054100     Document Type: Article

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