Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnants N 132D

arXiv:2610.11606 · astro-ph.HE · Submitted 2026-10-08 · Read on arXiv

astro-ph.HE

Submitted: 2026-10-08

Updated: 2026-10-08

Terminology

• Large Magellanic Cloud — 4× in this paper
• Trace — 3× in this paper · explained in 2 episodes
• Australia Telescope National Facility — 2× in this paper
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Atacama Large Millimeter Array — 1× in this paper
• Australia Telescope Compact Array — 1× in this paper
• Compact Array Broadband Back-end — 1× in this paper
• Consistency — 1× in this paper · explained in 3 episodes
• Cosmic Ray — 1× in this paper
• Hubble Space Telescope — 1× in this paper

Sources

• A distance to the Large Magellanic Cloud that is precise to one per cent
• The population of X-ray supernova remnants in the Large Magellanic Cloud
• Statistical Analysis of Supernova Remnants in the Large Magellanic Cloud
• New ASKAP Radio Supernova Remnants and Candidates in the Large Magellanic Cloud
• The Transition from Young to Middle-aged Supernova Remnants: Thermal and Nonthermal Aspects of SNR N132D
• LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV
• The 3D Structure of N132D in the LMC: A Late-Stage Young Supernova Remnant
• Three-Dimensional Kinematic Reconstruction of the Optically-Emitting, High-Velocity, Oxygen-Rich Ejecta of Supernova Remnant N132D
• The Magellanic Mopra Assessment (MAGMA). I. The Molecular Cloud Population of the Large Magellanic Cloud
• ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
• A retrospective view of Miriad
• The MeerKAT 1.3 GHz Survey of the Large Magellanic Cloud
• A Catalogue of Radio Supernova Remnants and Candidate Supernova Remnants in the EMU/POSSUM Galactic Pilot Field
• Teleios (G305.4-2.2) -- the mystery of a perfectly shaped new Galactic supernova remnant
• Faraday Rotation Measure Synthesis
• Radio Emission from Interstellar Shocks: Young Type Ia Supernova Remnants and the Case of N 103B in the Large Magellanic Cloud
• Faraday Rotation Observations of Magnetic Fields in galaxy Clusters
• Modified equipartition calculation for supernova remnants
• Modified equipartition calculation for supernova remnants. Cases \alpha =0.5 and \alpha =1
• On the foundation of equipartition in supernova remnants

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