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https://research.matf.bg.ac.rs/handle/123456789/2785| Title: | Numerical Code for Fitting Radial Emission Profile of a Shell Supernova Remnant | Authors: | Arbutina, Bojan Opsenica, Slobodan |
Affiliations: | Astronomy | Issue Date: | 2012 | Rank: | M63 | Publisher: | Beograd : Astronomska opservatorija | Related Publication(s): | Proceedings of the 16th National Conference of Astronomers of Serbia | Journal: | Publications of the Astronomical observatory Belgrade | Conference: | National Conference of Serbian Astronomers (16 ; 2011 ; Beograd) | Abstract: | 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. |
URI: | https://research.matf.bg.ac.rs/handle/123456789/2785 |
| Appears in Collections: | Research outputs |
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