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Size distribution of SNRs and the ISM

Published online by Cambridge University Press:  05 March 2015

Abdul I. Asvarov
Abdul I. Asvarov*
Affiliation:
Institute of Physics, Baku AZ1143, Azerbaijan Republic. email: asvarov@physics.ab.az
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Abstract

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Based on the very general assumptions on evolution, we have modeled the statistics of SNRs evolving at various initial and environmental conditions. The method is applied to M33, for which the value of the filling factor of the hot phase of the ISM is estimated to be ~ 10%.

Keywords

SNRs(ISM:) supernova remnantsgalaxies: M33
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 616
Copyright
Copyright © International Astronomical Union 2015 

References

Long, K. S., Blair, W. P., Winkler, P. F., et al. 2010, ApJS 187, 495CrossRefGoogle Scholar