A Statistical Analysis of Galactic Radio Supernova Remnants

TL;DR

This paper provides a comprehensive statistical analysis of 390 Galactic radio supernova remnants, examining their physical parameters, distribution, and the accuracy of distance estimation methods, offering new insights into their properties and Galactic distribution.

Contribution

It offers a revised catalog of SNRs with detailed statistical analysis and evaluates the accuracy of the $\Sigma$-D relation for distance estimation.

Findings

Average SNR diameter is 30.5 pc with a standard deviation of 25.4 pc.

Estimated supernova birth rate aligns within 2σ of accepted values.

No correlation between spectral indices and other SNR parameters.

Abstract

We present an revised table of 390 Galactic radio supernova remnants (SNRs) and their basic parameters. Statistical analyses are performed on SNR diameters, ages, spectral indices, Galactic heights and spherical symmetries. Furthermore, the accuracy of distances estimated using the $\Sigma$-D relation is examined. The arithmetic mean of the Galactic SNR diameters is $30.5$ pc with standard error $1.7$ pc and standard deviation $25.4$ pc. The geometric mean and geometric standard deviation factor of Galactic SNR diameters is $21.9$ pc and $2.4$, respectively. We estimate ages of 97 SNRs and find that the supernova (SN) birth rate to be lower than, but within $2\sigma$ of currently accepted values for SN birth rate. The mean spectral index of shell-type SNRs is $-0.51 \pm 0.01$ and no correlations are found between spectral indices and the SNR parameters of molecular cloud (MC) association, SN type, diameter, Galactic height and surface brightness. The Galactic height distribution of SNRs is best described by an exponential distribution with a scale height of $48 \pm 4$ pc. The spherical symmetry measured by the ovality of radio SNRs is not correlated to any other SNR parameters considered here or to explosion type.