scholarly journals Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning‐Front Propagation

1999 ◽  
Vol 125 (2) ◽  
pp. 439-462 ◽  
Author(s):  
Koichi Iwamoto ◽  
Franziska Brachwitz ◽  
Ken’ichi Nomoto ◽  
Nobuhiro Kishimoto ◽  
Hideyuki Umeda ◽  
...  
Keyword(s):  
Front Propagation ◽  
Type Ia Supernovae ◽  
Burning Front ◽  
Type Ia ◽  
Ia Supernovae

Hard X‐Rays and Gamma Rays from Type Ia Supernovae

1998 ◽  
Vol 492 (1) ◽  
pp. 228-245 ◽  
Author(s):  
P. Hoflich ◽  
J. C. Wheeler ◽  
A. Khokhlov
Keyword(s):  
Gamma Rays ◽  
Type Ia Supernovae ◽  
X Rays ◽  
Type Ia ◽  
Ia Supernovae

scholarly journals Gravitational Collapse versus Thermonuclear Explosion of Degenerate Stellar Cores

1994 ◽  
Vol 147 ◽  
pp. 186-213
Author(s):  
J. Isern ◽  
R. Canal
Keyword(s):  
Neutron Star ◽  
White Dwarfs ◽  
Light Curves ◽  
Type Ia Supernovae ◽  
Radioactive Elements ◽  
Border Line ◽  
Thermonuclear Explosion ◽  
Type Ia ◽  
Γ Rays ◽  
Ia Supernovae

AbstractIn this paper we review the behavior of growing stellar degenerate cores. It is shown that ONeMg white dwarfs and cold CO white dwarfs can collapse to form a neutron star. This collapse is completely silent since the total amount of radioactive elements that are expelled is very small and a burst of γ-rays is never produced. In the case of an explosion (always carbonoxygen cores), the outcome fits quite well the observed properties of Type Ia supernovae. Nevertheless, the light curves and the velocities measured at maximum are very homogeneous and the diversity introduced by igniting at different densities is not enough to account for the most extreme cases observed. It is also shown that a promising way out of this problem could be the He-induced detonation of white dwarfs with different masses. Finally, we outline that the location of the border line which separetes explosion from collapse strongly depends on the input physics adopted.

scholarly journals A Novel Color Parameter as a Luminosity Calibrator for Type Ia Supernovae

2005 ◽  
Vol 620 (2) ◽  
pp. L87-L90 ◽  
Author(s):  
Xiaofeng Wang ◽  
Lifan Wang ◽  
Xu Zhou ◽  
Yu-Qing Lou ◽  
Zongwei Li
Keyword(s):  
Type Ia Supernovae ◽  
Color Parameter ◽  
Type Ia ◽  
Ia Supernovae

scholarly journals Kernel PCA for Type Ia supernovae photometric classification

2013 ◽  
Vol 430 (1) ◽  
pp. 509-532 ◽  
Author(s):  
E. E. O. Ishida ◽  
R. S. de Souza
Keyword(s):  
Type Ia Supernovae ◽  
Kernel Pca ◽  
Type Ia ◽  
Ia Supernovae

scholarly journals WHITE DWARF/M DWARF BINARIES AS SINGLE DEGENERATE PROGENITORS OF TYPE Ia SUPERNOVAE

2012 ◽  
Vol 758 (2) ◽  
pp. 123 ◽  
Author(s):  
J. Craig Wheeler
Keyword(s):  
White Dwarf ◽  
Type Ia Supernovae ◽  
Type Ia ◽  
Ia Supernovae ◽  
M Dwarf

scholarly journals CONSTRAINTS ON SHALLOW56Ni FROM THE EARLY LIGHT CURVES OF TYPE Ia SUPERNOVAE

2014 ◽  
Vol 784 (1) ◽  
pp. 85 ◽  
Author(s):  
Anthony L. Piro ◽  
Ehud Nakar
Keyword(s):  
Light Curves ◽  
Type Ia Supernovae ◽  
Type Ia ◽  
Ia Supernovae

Recurrent Novae as a Progenitor System of Type Ia Supernovae. I. RS Ophiuchi Subclass: Systems with a Red Giant Companion

2001 ◽  
Vol 558 (1) ◽  
pp. 323-350 ◽  
Author(s):  
Izumi Hachisu ◽  
Mariko Kato
Keyword(s):  
Type Ia Supernovae ◽  
Type Ia ◽  
Red Giant ◽  
Ia Supernovae

scholarly journals Spectral diversity of Type Ia supernovae

2006 ◽  
Vol 370 (2) ◽  
pp. 933-940 ◽  
Author(s):  
J. B. James ◽  
T. M. Davis ◽  
B. P. Schmidt ◽  
A. G. Kim
Keyword(s):  
Type Ia Supernovae ◽  
Type Ia ◽  
Ia Supernovae

scholarly journals Artificial neural network for constructing type Ia supernovae spectrum evolution model

2018 ◽  
Vol 97 (12) ◽  
Author(s):  
Qiao-Bin Cheng ◽  
Chao-Jun Feng ◽  
Xiang-Hua Zhai ◽  
Xin-Zhou Li
Keyword(s):  
Neural Network ◽  
Artificial Neural Network ◽  
Evolution Model ◽  
Type Ia Supernovae ◽  
Type Ia ◽  
Artificial Neural ◽  
Ia Supernovae
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