scholarly journals CGRO/OSSE observations of the Cassiopeia A Supernova remnant

1995 ◽  
Vol 444 ◽  
pp. 244 ◽  
Author(s):  
L.-S. The ◽  
M. D. Leising ◽  
D. D. Clayton ◽  
W. N. Johnson ◽  
R. L. Kinzer ◽  
...  
Nature ◽  
2009 ◽  
Vol 462 (7269) ◽  
pp. 71-73 ◽  
Author(s):  
Wynn C. G. Ho ◽  
Craig O. Heinke

2019 ◽  
Vol 874 (1) ◽  
pp. 98 ◽  
Author(s):  
Xiao Zhang ◽  
Siming Liu

1994 ◽  
Author(s):  
L.-S. The ◽  
D. D. Clayton ◽  
M. D. Leising ◽  
W. N. Johnson ◽  
J. D. Kurfess ◽  
...  

1979 ◽  
Vol 83 ◽  
pp. 357-365
Author(s):  
Susan A. Lamb

Observations of the chemical abundances in young supernova remnants may be used, in some circumstances, to place constraints on the evolution of the progenitor stars. For example, if a progenitor was massive (M > 10 M⊙), the presence of high 14N/1H ratios (that is, more than five time the solar value) in the supernova remnant can imply that substantial mass loss took place during the star's early evolution, that is, while it was an early-type supergiant.


2013 ◽  
Vol 779 (2) ◽  
pp. 117 ◽  
Author(s):  
Yajie Yuan ◽  
Stefan Funk ◽  
Gülauger Jóhannesson ◽  
Joshua Lande ◽  
Luigi Tibaldo ◽  
...  

Science ◽  
2005 ◽  
Vol 308 (5728) ◽  
pp. 1604-1606 ◽  
Author(s):  
O. Krause

2010 ◽  
Vol 719 (2) ◽  
pp. 1553-1564 ◽  
Author(s):  
B. Sibthorpe ◽  
P. A. R. Ade ◽  
J. J. Bock ◽  
E. L. Chapin ◽  
M. J. Devlin ◽  
...  

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