Supernova Remnants

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Supernovae Remnants

Supernova explosions have a very profound impact on the Interstellar Medium (ISM), both as sources of mechanical energy and heavy elements. Supernova Remnants (SNRs) provide information about these issues and can be observed as high-energy X-ray sources. The interaction of high velocity ejecta with the ISM generates very high temperatures, giving rise to line emission from heavy elements. By studying the spatial distribution of elements, one can gain insight into nucleosynthesis in the progenitor and the geometry of the explosions. SNRs are also possible sites of cosmic ray acceleration.    [Ref  4]


 
1E 0102.9-7219 
 
30 Dor 
 
30 Dor 
 
30 Dor C 
 
3C 58 
 
3C391 
 
CAS A 
 
Cas A 
 
CAS A 
 
Crab Nebula 
 
Crab Nebula 
 
Crab Nebula 
 
Cygnus Loop 
 
G350.1-0.3 
 
HESS J1731-347 
 
IC 443 
 
IC443 
 
IC443 
 
IC443 
 
Kepler SNR 
 
Kesteven 79 
 
LMC RASS 0203 
 
Puppis A 
 
Puppis A 
 
RCW 103 

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