SPHGal: Smoothed particle hydrodynamics with improved accuracy for galaxy simulations

Monthly Notices of the Royal Astronomical Society

Volumn 443, Issue 2, 2014, Pages 1173-1191

  Hu, Chia Yu ^a   Naab, Thorsten ^a   Walch, Stefanie ^a,b   Moster, Benjamin P ^a,c   Oser, Ludwig ^d  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF COLOGNE   (Germany)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d Columbia University ^*  (United States)

Author keywords

Galaxies: evolution; Galaxies: ISM; Galaxies: spiral; Intergalactic medium; Methods: numerical

Indexed keywords

ENTROPY; GALAXIES; MIXING; NUMERICAL METHODS; STARS; VISCOSITY;

ARTIFICIAL VISCOSITY; FLUID MIXING; GALAXIES: ISM; GALAXIES: SPIRALS; GALAXY EVOLUTION; GALAXY SIMULATIONS; INTERGALACTIC MEDIUM; METHOD: NUMERICAL; SMOOTHED PARTICLE HYDRODYNAMICS; STAR FORMATION RATES;

HYDRODYNAMICS;

EID: 84905665614     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu1187     Document Type: Article

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