Size distribution of SNRs and the ISM
Abstract
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%.
- Publication:
-
Highlights of Astronomy
- Pub Date:
- March 2015
- DOI:
- 10.1017/S1743921314012459
- Bibcode:
- 2015HiA....16..616A
- Keywords:
-
- SNRs;
- (ISM:) supernova remnants;
- galaxies: M33