A localised subgrid scale model for fluid dynamical simulations in astrophysics II. Application to type la supernovae

Astronomy and Astrophysics

Volumn 450, Issue 1, 2006, Pages 283-294

  Schmidt, W ^a,b   Niemeyer, J C ^a   Hillebrandt, W ^b   Ropke F K ^b  

^a UNIVERSITY OF WÜRZBURG   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Convection; Hydrodynamics; Methods: numerical; Stars: supernovae: general; Turbulence

Indexed keywords

COMPUTER SIMULATION; ENERGY DISSIPATION; ENERGY TRANSFER; FLUID DYNAMICS; HEAT CONVECTION; HYDRODYNAMICS; SPACE APPLICATIONS; TURBULENCE; TURBULENT FLOW;

BURNING REGIONS; METHODS: NUMERICAL; STARS: SUPERNOVAE: GENERAL; TURBULENT VELOCITY;

ASTROPHYSICS;

EID: 33645835717     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20053618     Document Type: Article

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