Numerical code for fitting radial emission profile of a shell supernova remnant: Application

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 shel...

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Bibliographic Details
Main Authors: Opsenica Slobodan, Arbutina Bojan
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2011-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2011/1450-698X1183077O.pdf