Supernova Remnants In The Magellanic Clouds
Miroslav D. Filipovi\'c, Luke M. Bozzetto
TL;DR
This paper presents a comprehensive study of 108 supernova remnants in the Magellanic Clouds, analyzing their properties and including notable Type Ia SNRs, to enhance understanding of SNR populations in galaxies.
Contribution
It provides the most complete catalog of SNRs in any galaxy and analyzes their size and spectral index distributions, including insights into Type Ia supernova remnants.
Findings
Most complete sample of SNRs in any galaxy
Analysis of size and spectral index distributions
Highlights of 12 Type Ia SNRs in the LMC
Abstract
We present initial results of an ongoing study of the supernova remnants (SNRs) and candidates in the Magellanic Clouds. Some 108 objects in both Clouds are considered to be either an SNR or a reliable candidate. This represents the most complete sample of known SNRs in any galaxy. therefore, this study allows us to study SNR population properties such as the size and spectral index distribution. Here, we also show 12 known Large Magellanic Cloud SNRs from type Ia SN explosions and briefly comment on their importance.
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