A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence

Monthly Notices of the Royal Astronomical Society

Volumn 406, Issue 3, 2010, Pages 1659-1674

  Price, Daniel J ^a   Federrath, Christoph ^a,b,c  

^a MONASH UNIVERSITY   (Australia)

^b UNIVERSITY OF HEIDELBERG   (Germany)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Hydrodynamics; ISM: general; Methods: numerical; Shock waves; Stars: formation; Turbulence

Indexed keywords

AERODYNAMICS; CODES (SYMBOLS); DISTRIBUTION FUNCTIONS; HYDRODYNAMICS; MACH NUMBER; NUMERICAL METHODS; POWER SPECTRUM; PROBABILITY DENSITY FUNCTION; STATISTICS; TURBULENCE MODELS; VELOCITY;

GRID CELLS; GRID CODES; HIGH MACH NUMBER; HYDRODYNAMIC CODES; ISM:GENERAL; METHOD: NUMERICAL; POWER-SPECTRA; SHOCK-WAVES; SMOOTHED PARTICLE HYDRODYNAMICS; STARS FORMATION;

SHOCK WAVES;

EID: 77955255782     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16810.x     Document Type: Article

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