Bojan Arbutina, Slobodan Opsenica
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.
View original:
http://arxiv.org/abs/1201.0855
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