SEREN - A new SPH code for star and planet formation simulations: Algorithms and tests

Astronomy and Astrophysics

Volumn 529, Issue , 2011, Pages

  Hubber, D A ^a,b,c   Batty, C P ^b   McLeod, A ^b,d   Whitworth, A P ^b  

^a UNIVERSITY OF SHEFFIELD   (United Kingdom)

^b CARDIFF UNIVERSITY   (United Kingdom)

^c UNIVERSITY OF OSLO   (Norway)

^d ASTRONOMICAL INSTITUTE   (Czech Republic)

Author keywords

hydrodynamics; methods: numerical; stars: formation

Indexed keywords

BAROTROPIC EQUATION; COOLING RADIATION; ENERGY EQUATION; FORTRAN; GRAVITATIONAL ACCELERATIONS; HERMITE; METHODS: NUMERICAL; N-BODY SIMULATION; PLANET FORMATION; PROTOSTARS; SMOOTHED PARTICLE HYDRODYNAMICS; SPH CODE; STAR CLUSTERS; STARS: FORMATION; THERMAL PHYSICS; TIME STEP; TIME-STEPPING SCHEMES;

ALGORITHMS; APPLICATION PROGRAMMING INTERFACES (API); EQUATIONS OF STATE; FLUID DYNAMICS; HYDRODYNAMICS; NUMERICAL METHODS;

STARS;

EID: 79953060636     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014949     Document Type: Article

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