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27 April 2024
 
  » arxiv » 2210.05090

 Article overview



New ASKAP Radio Supernova Remnants and Candidates in the Large Magellanic Cloud
Luke M. Bozzetto ; Miroslav D. Filipović ; H. Sano ; R. Z. E. Alsaberi ; L. A. Barnes ; I. S. Bojičić ; R. Brose ; L. Chomiuk ; E. J. Crawford ; S. Dai ; M. Ghavam ; F. Haberl ; T. Hill ; A. M. Hopkins ; A. Ingallinera ; T. Jarrett ; P. J. Kavanagh ; B. S. Koribalski ; R. Kothes ; D. Leahy ; E. Lenc ; I. Leonidaki ; P. Maggi ; C. Maitra ; C. Matthew ; J. L. Payne ; C. M. Pennock ; S. Points ; W. Reid ; S. Riggi ; G. Rowell ; M. Sasaki ; S. Safi-Harb ; J. Th. van Loon ; N. F. H. Tothill ; D. Urošević ; F. Zangrandi ;
Date 11 Oct 2022
AbstractWe present a new Australian Square Kilometre Array Pathfinder (ASKAP) sample of 14 radio Supernova Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). This new sample is a significant increase to the known number of older, larger and low surface brightness LMC SNRs. We employ a multi-frequency search for each object and found possible traces of optical and occasionally X-ray emission in several of these 14 SNR candidates. One of these 14 SNR candidates (MCSNR J0522-6543) has multi-frequency properties that strongly indicate a bona fide SNR. We also investigate a sample of 20 previously suggested LMC SNR candidates and confirm the SNR nature of MCSNR J0506-6815. We detect lower surface brightness SNR candidates which were likely formed by a combination of shock waves and strong stellar winds from massive progenitors (and possibly surrounding OB stars). Some of our new SNR candidates are also found in a lower density environments in which SNe type Ia explode inside a previously excavated interstellar medium (ISM).
Source arXiv, 2210.05090
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