scholarly journals Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J

Nature ◽  
2014 ◽  
Vol 512 (7515) ◽  
pp. 406-408 ◽  
Author(s):  
E. Churazov ◽  
R. Sunyaev ◽  
J. Isern ◽  
J. Knödlseder ◽  
P. Jean ◽  
...  
1999 ◽  
Vol 514 (2) ◽  
pp. 844-855 ◽  
Author(s):  
A. Finoguenov ◽  
C. Jones ◽  
W. Forman ◽  
L. David

2009 ◽  
Vol 697 (1) ◽  
pp. 380-408 ◽  
Author(s):  
X. Wang ◽  
W. Li ◽  
A. V. Filippenko ◽  
R. J. Foley ◽  
R. P. Kirshner ◽  
...  

2010 ◽  
Vol 410 (1) ◽  
pp. 585-611 ◽  
Author(s):  
Jeffrey M. Silverman ◽  
Mohan Ganeshalingam ◽  
Weidong Li ◽  
Alexei V. Filippenko ◽  
Adam A. Miller ◽  
...  
Keyword(s):  
Type Ia ◽  

2016 ◽  
Vol 466 (1) ◽  
pp. 884-891 ◽  
Author(s):  
David Cinabro ◽  
Daniel Scolnic ◽  
Richard Kessler ◽  
Ashley Li ◽  
Jake Miller
Keyword(s):  

2011 ◽  
Vol 63 (4) ◽  
pp. L31-L35 ◽  
Author(s):  
Xiang Cun Meng ◽  
Zhong Mu Li ◽  
Wu Ming Yang

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.


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