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SUPERNOVA REMNANTS IN THE MAGELLANIC CLOUDS

  • BOZZETTO, LUKE M. (University of Western Sydney) ;
  • FILIPOVIC, MIROSLAV D. (University of Western Sydney) ;
  • HABERL, FRANK (Max-Planck-Institut fur extraterrestrische Physik) ;
  • SASAKI, MANAMI (Institut fur Astronomie und Astrophysik Tubingen) ;
  • KAVANAGH, PATRICK (Institut fur Astronomie und Astrophysik Tubingen) ;
  • MAGGI, PIERRE (Max-Planck-Institut fur extraterrestrische Physik) ;
  • UROSEVIC, DEJAN (Department of Astronomy, Faculty of Mathematics, University of Belgrade) ;
  • STURM, RICHARD (Max-Planck-Institut fur extraterrestrische Physik)
  • Received : 2014.11.30
  • Accepted : 2015.06.30
  • Published : 2015.09.30
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Abstract

We present an ongoing study of the complete sample of supernova remnants (SNRs) and candidates in the Magellanic Clouds. 108 objects in both Clouds are considered to be either SNR or reliable candidates. This represents the most complete sample of all known SNRs in any galaxy. It therefore allows us to study SNR population properties such as the age-diameter (Age-D) relation. Here, we show that this Age-D relation is strongly dependant on the local environment in which SNRs are residing.

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References

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