Theoretical light curves for deflagration models of type la supernova

Astronomy and Astrophysics

Volumn 453, Issue 1, 2006, Pages 229-240

  Blinnikov, S I ^a,b   Ropke F K ^a,c   Sorokina, E I ^a,d   Gieseler, M ^a   Reinecke, M ^a   Travaglio, C ^e   Hillebrandt, W ^a   Stritzinger, M ^a,f  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b INSTITUTE FOR THEORETICAL AND EXPERIMENTAL PHYSICS   (Russian Federation)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d MOSCOW STATE UNIVERSITY   (Russian Federation)

^e OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^f UNIVERSITY OF COPENHAGEN   (Denmark)

Author keywords

Hydrodynamics; Methods: numerical; Radiative transfer; Stars: supernovae: general

Indexed keywords

BOLOMETERS; COMPUTER SIMULATION; GALAXIES; HYDRODYNAMICS; KINETIC ENERGY; MATHEMATICAL MODELS; NUMERICAL METHODS; RADIOACTIVE ELEMENTS; THEOREM PROVING; THERMONUCLEAR REACTIONS; THREE DIMENSIONAL;

ARNETT'S RULE; MATERIAL VELOCITY; RADIATIVE TRANSFER; STAR SUPERNOVAE;

ASTROPHYSICS;

EID: 33744976973     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054594     Document Type: Article

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