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:	ISM: supernova remnants radio continuum: ISM methods: numerical ISM: individual objects: G17.8-2.6, G54.4-0.3, G127.1+0.5, G132.7+1.3, G332.0+0.2
Online Access:	http://www.doiserbia.nb.rs/img/doi/1450-698X/2011/1450-698X1183077O.pdf

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