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A modified theoretical Σ − D relation for supernova remnants: II. The case of variable temperature within the supernova remnant

In this preliminary report a modification of the theoretical Σ − D relation for supernova remnants (SNRs) in the adiabatic expansion phase is presented in another way. As in Paper I, this modification is based on the convolution procedure. The relation first derived by Shklovsky is convoluted with t...

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Autori principali: Urošević Dejan V., Đurić N., Pannuti T.
Natura: Artigo
Lingua:Inglês
Pubblicazione: Astronomical Observatory, Department of Astronomy, Belgrade 2003-01-01
Serie:Serbian Astronomical Journal
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Accesso online:http://www.doiserbia.nb.rs/img/doi/1450-698X/2003/1450-698X0366067U.pdf
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