Properties of supernova remnants in SIGNALS galaxies -- I . NGC 6822 and M33

TL;DR

This study analyzes the kinematic properties of supernova remnants in NGC 6822 and M33 using SITELLE data, introducing new identification methods based on emission line ratios and velocity dispersion.

Contribution

It presents a novel scheme for identifying extragalactic SNRs by combining [SII]/Hα ratios and velocity dispersion, including a new parameter to improve SNR detection.

Findings

Over 90% of SNRs have [SII]/Hα > 0.4

86% of SNRs show significant velocity dispersion

Complex velocity structures observed in some SNRs

Abstract

We present a spatially resolved study of the kinematical properties of known supernova remnants (SNRs) in the nearest galaxies of the SIGNALS survey, namely NGC 6822 (one object) and M33 (163 objects), based on data obtained with the SITELLE Imaging Fourier Transform Spectrometer (iFTS) at the Canada-France-Hawaii Telescope. The purpose of this paper is to provide a better scheme of identification for extragalactic SNRs and, in particular, to distinguish between HII regions and SNRs. For that we have used diagrams which involve both the [SII]/H$\alpha$ ratio and the velocity dispersion ($\sigma$). We also introduce a new parameter, $\xi = {[SII] \over H\alpha} \times \sigma$, which enhances still the contrast between SNRs and the rest of the ionised gas. More than 90\% of the SNRs in our entire sample show an integrated [SII]/H$\alpha$ ratio larger than the canonical value (0.4). 86\% of the SNRs present in our field show a significant velocity dispersion. The spectral resolution of our observations allows us to observe the complex velocity structure of some SNRs.