Affiliation:
1. Department of Astronomy, Faculty of Mathematics, Belgrade
Abstract
We present IDL (Interactive Data Language) codes for fitting a theoretical
emission profile of a shell supernova remnant (SNR) to the mean profile of an
SNR obtained from radio observations. Two considered theoretical models are:
1) a shell with constant emissivity and 2) a synchrotron shell with radially
aligned magnetic field. The codes were applied to several observed supernova
remnants. Good results are obtained in five considered cases, which justify
the use of our code for remnants that are bright (so that observational
errors are not large) and spherically symmetric enough.
Publisher
National Library of Serbia
Subject
Astronomy and Astrophysics
Cited by
2 articles.
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