LMC N132D: a mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV

<p><strong>Context</strong> Supernova remnants (SNRs) are commonly thought to be the dominant sources of Galactic cosmic rays up to the knee of the cosmic-ray spectrum at a few PeV. Imaging Atmospheric Cherenkov Telescopes have revealed young SNRs as very-high-energy (VHE, >...

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Bibliographic Details
Main Authors:	Abdalla, H, Aharonian, F, Benkhali, FA, Anguner, EO, Arcaro, C, Armand, C, Armstrong, T, Ashkar, H, Backes, M, Baghmanyan, V, Martins, VB, Barnacka, A, Barnard, M, Batzofin, R, Becherini, Y, Berge, D, Bernloehr, K, Bi, B, Boettcher, M, Boisson, C, Bolmont, J, de Lavergne, MDB, Breuhaus, M, Brose, R, Brun, F, Bulik, T, Bylund, T, Cangemi, F, Caroff, S, Casanova, S, Catalano, J, Chambery, P, Chand, T, Chen, A, Cotter, G, Curylo, M, Mbarubucyeye, JD, Davids, ID, Davies, J, Devin, J, Djannati-Atai, A, Dmytriiev, A, Donath, A, Doroshenko, V, Dreyer, L, Du Plessis, L, Duffy, C, Egberts, K, Einecke, S
Other Authors:	H.E.S.S. Collaboration
Format:	Journal article
Language:	English
Published:	EDP Sciences 2021

LMC N132D: a mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV

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