SIMBAD references

2005MNRAS.360...76A - Mon. Not. R. Astron. Soc., 360, 76-80 (2005/June-2)

Σ-D relation for supernova remnants and its dependence on the density of the interstellar medium.

ARBUTINA B. and UROSEVIC D.

Abstract (from CDS):

During the last couple of decades of work on the Σ-D (radio surface brightness to diameter) relation for supernova remnants (SNRs), it has been generally accepted that no single Σ-D relation can be constructed for all SNRs. However, it may still be possible to construct the relations for some classes of SNRs. In our previous paper we analysed Σ-D relation(s) for remnants in the dense environments of molecular clouds. The aim of this paper is to examine, in the same context, a class of oxygen-rich SNRs, and to extend the analysis to remnants evolving in lower-density interstellar media, namely Balmer-dominated SNRs. We have obtained good relations with certain similarities to our previous findings - similarities that emphasize, again, the role of ambient density in the evolution of SNRs.

Abstract Copyright: 2005 RAS

Journal keyword(s): methods: statistical - supernova remnants - radio continuum: ISM

CDS comments: P.78 : IKT 19 is a misprint for IKT 25.

Simbad objects: 24

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2021.03.04-17:32:58

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