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

H.E.S.S. Collaboration, Abdalla, H., Aharonian, F., Ait Benkhali, F., Angüner, E. O., Arcaro, C., et al. (2021). LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV. Astronomy and Astrophysics, 655: A7. doi:10.1051/0004-6361/202141486.

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H.E.S.S. Collaboration, Author              
Abdalla, H., Author
Aharonian, F.1, Author           
Ait Benkhali, F.1, Author           
Angüner, E. O., Author
Arcaro, C., Author
Armand, C., Author
Armstrong, T., Author
Ashkar, H., Author
Backes, M., Author
Baghmanyan, V., Author
Barbosa Martins, V. , Author
Barnacka, A., Author
Barnard, M., Author
Batzofin, R., Author
Becherini, Y., Author
Berge, D., Author
Bernlöhr, K.1, Author           
Bi, B., Author
Böttcher, M., Author
Boisson, C., AuthorBolmont, J., AuthorBony de de Lavergne, M. , AuthorBreuhaus, M.1, Author           Brose, R., AuthorBrun, F., AuthorBulik, T., AuthorBylund, T., AuthorCangemi, F., AuthorCaroff, S., AuthorCasanova, S., AuthorCatalano, J., AuthorChambery, P., AuthorChand, T., AuthorChen, A., AuthorCotter, G., AuthorCuryło, M., AuthorDamascene Mbarubucyeye, J. , AuthorDavids, I. D., AuthorDavies, J., AuthorDevin, J., AuthorDjannati-Ataï, A., AuthorDmytriiev, A., AuthorDonath, A.1, Author           Doroshenko, V., AuthorDreyer, L., AuthorDu Plessis, L. , AuthorDuffy, C., AuthorEgberts, K., AuthorEinecke, S., AuthorErnenwein, J.-P., AuthorFegan, S., AuthorFeijen, K., AuthorFiasson, A., AuthorFichet de Clairfontaine, G. , AuthorFontaine, G., AuthorLott, F., AuthorFüßling, M., AuthorFunk, S., AuthorGabici, S., AuthorGallant, Y. A., AuthorGiavitto, G., AuthorGiunti, L., AuthorGlawion, D., AuthorGlicenstein, J. F., AuthorGrondin, M.-H., AuthorHattingh, S., AuthorHaupt, M., AuthorHermann, G.1, Author           Hinton, J. A.1, Author           Hofmann, W.2, Author           Hoischen, C., AuthorHolch, T. L., AuthorHoller, M., AuthorHörbe, M., AuthorHorns, D., AuthorHuang, Zhiqiu3, Author           Huber, D., AuthorJamrozy, M., AuthorJankowsky, F., AuthorJoshi, V., AuthorJung-Richardt, I., AuthorKasai, E., AuthorKatarzyński, K., AuthorKatz, U., AuthorKhangulyan, D., AuthorKhélifi, B., AuthorKlepser, S., AuthorKluźniak, W., AuthorKomin, Nu., AuthorKonno, R., AuthorKosack, K., AuthorKostunin, D., AuthorKreter, M., AuthorKukec Mezek, G. , AuthorKundu, A., AuthorLamanna, G., AuthorLe Stum, S., AuthorLemière, A., AuthorLemoine-Goumard, M., AuthorLenain, J.-P., AuthorLeuschner, F., AuthorLevy, C., AuthorLohse, T., AuthorLuashvili, A., AuthorLypova, I., AuthorMackey, J., AuthorMajumdar, J., AuthorMalyshev, D., AuthorMalyshev, D., AuthorMarandon, V.1, Author           Marchegiani, P., AuthorMarcowith, A., AuthorMares, A., AuthorMartí-Devesa, G., AuthorMarx, R., AuthorMaurin, G., AuthorMeintjes, P. J., AuthorMeyer, M., AuthorMitchell, A.4, Author           Moderski, R., AuthorMohrmann, L., AuthorMontanari, A., AuthorMoore, C., AuthorMoulin, E., AuthorMuller, J., AuthorMurach, T., AuthorNakashima, K., Authorde Naurois, M., AuthorNayerhoda, A., AuthorNdiyavala, H., AuthorNiemiec, J., AuthorPriyana Noel, A. , AuthorO’Brien, P., AuthorOberholzer, L., AuthorOdaka, H., AuthorOhm, S., AuthorOlivera Nieto, L.1, Author           de Ona Wilhelmi, E. , AuthorOstrowski, M., AuthorPanny, S., AuthorPanter, M.1, Author           Parsons, R. D., AuthorPeron, G.1, Author           Pita, S., AuthorPoireau, V., AuthorProkhorov, D. A., AuthorProkoph, H., AuthorPühlhofer, G., AuthorPunch, M., AuthorQuirrenbach, A., AuthorReichherzer, P., AuthorReimer, A., AuthorReimer, O., AuthorRemy, Q.1, Author           Renaud, M., AuthorReville, B.3, Author           Rieger, F.1, Author           Romoli, C.1, Author           Rowell, G., AuthorRudak, B., AuthorRueda Ricarte, H. , AuthorRuiz-Velasco, E.1, Author           Sahakian, V., AuthorSailer, S.1, Author           Salzmann, H., AuthorSanchez, D. A., AuthorSantangelo, A., AuthorSasaki, M., AuthorSchäfer, J., AuthorSchüssler, F., AuthorSchutte, H. M., AuthorSchwanke, U., AuthorSenniappan, M., AuthorSeyffert, A. S., AuthorShapopi, J. N. S., AuthorShiningayamwe, K., AuthorSimoni, R., AuthorSinha, A., AuthorSol, H., AuthorSpecovius, A., AuthorSpencer, S., AuthorSpir-Jacob, M., AuthorStawarz, Ł., AuthorSteenkamp, R., AuthorStegmann, C., AuthorSteinmassl, S.1, Author           Steppa, C., AuthorSun, L., AuthorTakahashi, T., AuthorTanaka, T., AuthorTavernier, T., AuthorTaylor, A. M., AuthorTerrier, R., AuthorThiersen, J. H. E., AuthorThorpe-Morgan, C., AuthorTluczykont, M., AuthorTomankova, L., AuthorTsirou, M.3, Author           Tsuji, N., AuthorTuffs, R.1, Author           Uchiyama, Y., Authorvan der Walt, D. J., Authorvan Eldik, C., Authorvan Rensburg, C., Authorvan Soelen, B., AuthorVasileiadis, G., AuthorVeh, J., AuthorVenter, C., AuthorVincent, P., AuthorVink, J., AuthorVölk, H. J.5, Author           Wagner, S. J., AuthorWatson, J., AuthorHofmann, W.2, Author           White, R.1, Author           Wierzcholska, A., AuthorWong, Yu Wun, AuthorYassin, H., AuthorYusafzai, A., AuthorZacharias, M., AuthorZanin, R.1, Author           Zargaryan, D., AuthorZdziarski, A. A., AuthorZech, A., AuthorZhu, S. J., AuthorZmija, A., AuthorZouari, S., AuthorŻywucka, N., Author more..
Affiliations:
1Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society, ou_2074298              
2Prof. Werner Hofmann, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_3188608              
3Brian Reville, Astrophysical Plasma Theory (APT) - Max Planck Research Group, Junior Research Groups, MPI for Nuclear Physics, Max Planck Society, ou_3055242              
4Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
5Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907548              

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Free keywords: gamma rays: general / cosmic rays / ISM: supernova remnants
 MPINP: HESS - Abteilung Hinton
 Abstract: Context. 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, >100 GeV) gamma-ray sources, but for only a few SNRs the hadronic cosmic-ray origin of their gamma-ray emission is indisputably established. In all these cases, the gamma-ray spectra exhibit a spectral cutoff at energies much below 100 TeV and thus do not reach the PeVatron regime.

Aims. The aim of this work was to achieve a firm detection for the oxygen-rich SNR LMC N132D in the VHE gamma-ray domain with an extended set of data, and to clarify the spectral characteristics and the localization of the gamma-ray emission from this exceptionally powerful gamma-ray-emitting SNR.

Methods. We analyzed 252 h of High Energy Stereoscopic System (H.E.S.S.) observations towards SNR N132D that were accumulated between December 2004 and March 2016 during a deep survey of the Large Magellanic Cloud, adding 104 h of observations to the previously published data set to ensure a > 5σ detection. To broaden the gamma-ray spectral coverage required for modeling the spectral energy distribution, an analysis of Fermi-LAT Pass 8 data was also included.

Results. We unambiguously detect N132D at VHE with a significance of 5.7σ. We report the results of a detailed analysis of its spectrum and localization based on the extended H.E.S.S. data set. The joint analysis of the extended H.E.S.S and Fermi-LAT data results in a spectral energy distribution in the energy range from 1.7 GeV to 14.8 TeV, which suggests a high luminosity of N132D at GeV and TeV energies. We set a lower limit on a gamma-ray cutoff energy of 8 TeV with a confidence level of 95%. The new gamma-ray spectrum as well as multiwavelength observations of N132D when compared to physical models suggests a hadronic origin of the VHE gamma-ray emission.

Conclusions. SNR N132D is a VHE gamma-ray source that shows a spectrum extending to the VHE domain without a spectral cutoff at a few TeV, unlike the younger oxygen-rich SNR Cassiopeia A. The gamma-ray emission is best explained by a dominant hadronic component formed by diffusive shock acceleration. The gamma-ray properties of N132D may be affected by an interaction with a nearby molecular cloud that partially lies inside the 95% confidence region of the source position.

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 Dates: 2021-10-28
 Publication Status: Published online
 Pages: 13
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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: Les Ulis Cedex A France : EDP Sciences
Pages: - Volume / Issue: 655 Sequence Number: A7 Start / End Page: - Identifier: ISSN: 1432-0746
ISSN: 0004-6361
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1