scholarly journals Three‐dimensional Numerical Simulations of Rayleigh‐Taylor Unstable Flames in Type Ia Supernovae

2005 ◽  
Vol 632 (2) ◽  
pp. 1021-1034 ◽  
Author(s):  
M. Zingale ◽  
S. E. Woosley ◽  
C. A. Rendleman ◽  
M. S. Day ◽  
J. B. Bell
2009 ◽  
Vol 696 (2) ◽  
pp. 1491-1497 ◽  
Author(s):  
F. Ciaraldi-Schoolmann ◽  
W. Schmidt ◽  
J. C. Niemeyer ◽  
F. K. Röpke ◽  
W. Hillebrandt

2013 ◽  
Vol 438 (2) ◽  
pp. 1762-1783 ◽  
Author(s):  
Michael Fink ◽  
Markus Kromer ◽  
Ivo R. Seitenzahl ◽  
Franco Ciaraldi-Schoolmann ◽  
Friedrich K. Röpke ◽  
...  

2005 ◽  
Vol 437 (3) ◽  
pp. 983-995 ◽  
Author(s):  
C. Kozma ◽  
C. Fransson ◽  
W. Hillebrandt ◽  
C. Travaglio ◽  
J. Sollerman ◽  
...  

2004 ◽  
Vol 608 (2) ◽  
pp. 883-906 ◽  
Author(s):  
J. B. Bell ◽  
M. S. Day ◽  
C. A. Rendleman ◽  
S. E. Woosley ◽  
M. Zingale

2014 ◽  
Vol 444 (1) ◽  
pp. 350-351 ◽  
Author(s):  
Ivo R. Seitenzahl ◽  
Franco Ciaraldi-Schoolmann ◽  
Friedrich K. Röpke ◽  
Michael Fink ◽  
Wolfgang Hillebrandt ◽  
...  

2012 ◽  
Vol 429 (2) ◽  
pp. 1156-1172 ◽  
Author(s):  
Ivo R. Seitenzahl ◽  
Franco Ciaraldi-Schoolmann ◽  
Friedrich K. Röpke ◽  
Michael Fink ◽  
Wolfgang Hillebrandt ◽  
...  

2003 ◽  
Vol 208 ◽  
pp. 413-414
Author(s):  
Daisuke Kawata ◽  
Brad K. Gibson

We investigate the chemo-dynamical evolution of elliptical galaxies, to understand the origin of the mass-dependence of photometric properties such as the colour-magnitude relation (CMR). Our three-dimensional TREE N-body/SPH numerical simulation takes into account both Type II and Type Ia supernovae and follows the evolution of the abundances of several chemical elements. We derive the photometric properties of the simulation end-products and compare them with the observed CMR.


2002 ◽  
Vol 391 (3) ◽  
pp. 1167-1172 ◽  
Author(s):  
M. Reinecke ◽  
W. Hillebrandt ◽  
J. C. Niemeyer

2004 ◽  
Vol 606 (2) ◽  
pp. 1029-1038 ◽  
Author(s):  
J. B. Bell ◽  
M. S. Day ◽  
C. A. Rendleman ◽  
S. E. Woosley ◽  
M. Zingale

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