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https://research.matf.bg.ac.rs/handle/123456789/2991| Title: | Models of the magnetic field evolution in supernova remnants | Authors: | Vukotic, Branislav M Arbutina, Bojan Urošević, Dejan |
Affiliations: | Astronomy Astronomy |
Issue Date: | 2006 | Rank: | M63 | Publisher: | Beograd : Astronomska opservatorija | Related Publication(s): | Proceedings of the 14th National Conference of Astronomers of Serbia and Montenegro | Journal: | Publications of the Astronomical Observatory of Belgrade | Conference: | National Conference of Astronomers of Serbia and Montenegro (14 ; 2005 ; Beograd) | Abstract: | In this paper we present a brief discussion of the magnetic field (H) evolution in supernova remnant (SNRs). Evolution models generally assume H ∝ D−δ . Knowing δ would be particularly important in the study of the radio surface brightness to diameter (Σ − D) relation for SNRs, since it would allow us to compare different theoretical models for the radio evolution. |
URI: | https://research.matf.bg.ac.rs/handle/123456789/2991 |
| Appears in Collections: | Research outputs |
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