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

• 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
• ISSN: 1450-698X; 1820-9289

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.