Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mnras.360...76a&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 360, Issue 1, pp. 76-80.
Astronomy and Astrophysics
Astronomy
8
Methods: Statistical, Supernova Remnants, Radio Continuum: Ism
Scientific paper
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.
Arbutina Bojan
Urosević Dejan
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