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High energy gamma-ray detection of supernova remnants in the Large Magellanic Cloud

We present the results of a cluster search in the gamma-ray sky images of the Large Magellanic Cloud (LMC) region by means of the Minimum Spanning Tree (MST) and DBSCAN algorithms, at energies higher than 6 and 10 GeV, using 12 years of Fermi-LAT data. Several significant clusters were found, the majority of which associated with previously known gamma-ray sources. We confirm our previous detection of the Supernova Remnants N 49B and N 63A and found new significant clusters associated with the SNRs N 49, N 186D and N 44. These sources are among the brightest X-ray remnants in the LMC and corresponds to core-collapse supernovae interacting with dense HII regions, indicating that an hadronic origin of high energy photons is the most likely process.

preprint2022arXivOpen access
R. CampanaE. MassaroF. BocchinoM. MiceliS. OrlandoA. Tramacere
astro-ph.GAastro-ph.HE
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R. CampanaE. MassaroF. BocchinoM. MiceliS. OrlandoA. Tramacere

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