Numerical Code for Fitting Radial Emission Profile of a Shell Supernova Remnant

Details Numerical Code for Fitting Radial Emission Profile of a Shell Supernova Remnant Numerical Code for Fitting Radial Emission Profile of a Shell Supernova Remnant

2012-01-04

arxiv.org/abs/1201.0855v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

5 pages, 3 figures, XVI National Conference of Astronomers of Serbia, Belgrade, October 10-12, 2011

Scientific paper

Expressions for surface brightness distribution and for flux density have been theoretically derived in the case of two simple models of a shell supernova remnant. The models are: a homogenous optically thin emitting shell with constant emissivity and a synchrotron shell source with radial magnetic field. Interactive Data Language (IDL) codes for fitting theoretically derived emission profiles assuming these two models to mean profiles of shell supernova remnants obtained from radio observations have been written.

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