Non-spherical core collapse supernovae: I. Neutrino-driven convection, Rayleigh-Taylor instabilities, and the formation and propagation of metal clumps

Astronomy and Astrophysics

Volumn 408, Issue 2, 2003, Pages 621-649

  Kifonidis, K ^a   Plewa, T ^a,b,c   Janka, H Th ^a   Muller E ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^c UNIVERSITY OF CHICAGO   (United States)

Author keywords

Hydrodynamics; Instabilities; Nuclear reactions, nucleosynthesis abundances; Shock waves; Stars: supernovae: general

Indexed keywords

COMPUTER SIMULATION; ENTROPY; EXPLOSIONS; HYDRODYNAMICS; SHOCK WAVES;

STARS;

ASTROPHYSICS;

EID: 0141829736     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030863     Document Type: Article

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