scholarly journals Three-dimensional simulations of the interaction between Type Ia supernova ejecta and their main sequence companions

2012 ◽  
Vol 548 ◽  
pp. A2 ◽  
Author(s):  
Z. W. Liu ◽  
R. Pakmor ◽  
F. K. Röpke ◽  
P. Edelmann ◽  
B. Wang ◽  
...  
2006 ◽  
Vol 2 (14) ◽  
pp. 308-309
Author(s):  
Friedrich K. Röpke

AbstractKeeping up with ever more detailed observations, Type Ia supernova (SN Ia) explosion models have seen a brisk development over the past years. The aim is to construct a self-consistent picture of the physical processes in order to gain the predictive power necessary to answer questions arising from the application of SNe Ia as cosmological distance indicators. We review recent developments in modeling these objects focusing on three-dimensional simulations.


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

2006 ◽  
Vol 453 (1) ◽  
pp. 203-217 ◽  
Author(s):  
F. K. Röpke ◽  
M. Gieseler ◽  
M. Reinecke ◽  
C. Travaglio ◽  
W. Hillebrandt

2012 ◽  
Vol 8 (S289) ◽  
pp. 329-329
Author(s):  
Paul Ricker ◽  
Kuo-Chuan Pan ◽  
Ronald Taam

AbstractPopulation synthesis modeling of Type Ia supernova (SN Ia) progenitors suggests that multiple binary evolution channels may give rise to SNe Ia. Independently of the ignition mechanism, the type of progenitor system involved affects the circumstellar environment into which the explosion propagates, as well as the amount of solid angle blocked by the companion (for single-degenerate models). Using three-dimensional adaptive-mesh simulations of SNe Ia in binary systems, we discuss the effects of the progenitor system on the observable characteristics of SNe Ia and the impact of these effects on systematic errors in the use of SNe Ia as cosmic distance indicators.


2008 ◽  
Vol 681 (2) ◽  
pp. 1448-1457 ◽  
Author(s):  
G. C. Jordan IV ◽  
R. T. Fisher ◽  
D. M. Townsley ◽  
A. C. Calder ◽  
C. Graziani ◽  
...  

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