Fermi-LAT detects point-like gamma-ray emission from SNR B0453-685, with broadband modeling favoring an evolved PWN impacted by the SNR reverse shock and possible pulsar contribution below 5 GeV.
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Fermi-LAT Gamma-ray Emission Discovered from the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud
Fermi-LAT detects point-like gamma-ray emission from SNR B0453-685, with broadband modeling favoring an evolved PWN impacted by the SNR reverse shock and possible pulsar contribution below 5 GeV.