Studying the nature of the unidentified gamma-ray source HESS J1841−055 with the MAGIC telescopes

Acciari, V. A.; Bigongiari, C.; Dorner, D.; ́opez, R. J. Garcia L.; Sahakyan, N.; Strom, D.; Kubo, H.; Elsaesser, D.; Paneque, D.; Oka, T.; Verguilov, V.; Puljak, I.; Persic, M.; Suda, Y.; Truzzi, S.; Vazquez Acosta, M.; Bonnoli, G.; Hahn, A.; Doro, M.; Saha, L.; Manganaro, M.; Temnikov, P.; Carosi, R.; Fonseca, M. V.; Maneva, G.; Priyadarshi, C.; Font, L.; Miener, T.; Gasparyan, S.; Engels, A. Arbet; Jouvin, L.; D'Elia, V.; MAGIC Collaboration; Vanzo, G.; Depaoli, D.; Maraschi, L.; Barres de Almeida, U.; Schmidt, K.; Teshima, M.; Banerjee, B.; Miranda, J. M.; Saito, T.; Moretti, E.; Babic, A.; Karjalainen, M.; Hadasch, D.; Schleicher, B.; Prandini, E.; Inoue, S.; Bellizzi, L.; Mender, S.; Hoang, J.; Paoletti, R.; Busetto, G.; Bosnjak, Z.; Mariotti, M.; Fruck, C.; Berti, A.; Mirzoyan, R.; Hutten, M.; Zaric, D.; Sitarek, J.; Takahashi, M.; Stamerra, A.; Vitale, V.; Di Pierro, F.; Asano, K.; Giglietto, N.; Tosti, L.; Lindfors, E.; Satalecka, K.; Torres-Alba, N.; Lopez, M.; Nigro, C.; Delfino, M.; Otero-Santos, J.; Lopez-Coto, R.; Hrupec, D.; Mannheim, K.; De Angelis, A.; Antonelli, L. A.; Rhode, W.; Longo, F.; Godinovic, N.; Ferrara, G.; Ishio, K.; Makariev, M.; Molina, E.; Schweizer, T.; Donini, A.; Micanovic, S.; Ventura, S.; Spolon, A.; Bhattacharyya, W.; Noda, K.; Bernardos, M.; Lombardi, S.; Miceli, D.; Nishijima, K.; Tavecchio, F.; Paredes, J. M.; D'Amico, G.; Mazin, D.; Di Venere, L.; Da Vela, P.; Majumdar, P.; Garczarczyk, M.; Di Girolamo, T.; Suric, T.; Lopez-Oramas, A.; Contreras, J. L.; Leone, F.; Besenrieder, J.; Chilingarian, A.; Gaug, M.; de Oliveira Fraga, B. Machado; Palatiello, M.; Delgado Mendez, C.; Fallah Ramazani, V.; Moreno, V.; Ribo, M.; Cerruti, M.; BecerraGonzalez, J.; Munar-Adrover, P.; Loporchio, S.; Heckmann, L.; Rugliancich, A.; Sakurai, S.; Kajiwara, Y.; Strzys, M.; Dominis Prester, D.; Colombo, E.; Fattorini, A.; Bernardini, E.; De Lotto, B.; Righi, C.; Dazzi, F.; Iwamura, Y.; Blanch, O.; Barrio, 0J. A.; Snidaric, I.; Lamastra, A.; Delgado, J.; Vigorito, C. F.; van Scherpenberg, J.; Green, D.; Ansoldi, S.; Terzic, T.; Vovk, I.; Minev, M.; Chai, Y.; Bednarek, W.; Maggio, C.; Neustroev, V.; Nilsson, K.; Kobayashi, Y.; Fukami, S.; Rico, J.; Sobczynska, D.; Pavletic, L.; Kerszberg, D.; Biland, A.; Kushida, J.; Inada, T.; Covino, S.; Foffano, L.; Lelas, D.; Perennes, C.; Ceribella, G.; Cortina, J.; Cikota, S.; Ohtani, Y.; Colak, S. M.; Morcuende, D.; Prada Moroni, P. G.; Will, M.; Penil, P.; Herrera, J.; Mallamaci, M.; Baquero, A.; Nozaki, S.; Baack, D.; Giordano, F.; do Souto Espineira, E.; Moralejo, A.; Ninci, D.; Gliwny, P.; Martinez, M.

doi:10.1093/mnras/staa2135

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000452631 0247_ $$2doi$$a10.1093/mnras/staa2135
000452631 0247_ $$2INSPIRETeX$$aAcciari:2020khi
000452631 0247_ $$2inspire$$ainspire:1807981
000452631 0247_ $$2ISSN$$a0035-8711
000452631 0247_ $$2ISSN$$a1365-2966
000452631 0247_ $$2ISSN$$a1365-8711
000452631 0247_ $$2arXiv$$aarXiv:2007.09321
000452631 0247_ $$2altmetric$$aaltmetric:86154340
000452631 0247_ $$2WOS$$aWOS:000577137200089
000452631 0247_ $$2datacite_doi$$a10.3204/PUBDB-2020-04788
000452631 0247_ $$2openalex$$aopenalex:W3043638339
000452631 037__ $$aPUBDB-2020-04788
000452631 041__ $$aEnglish
000452631 082__ $$a520
000452631 088__ $$2arXiv$$aarXiv:2007.09321
000452631 1001_ $$0V.A.Acciari.2$$aAcciari, V. A.$$b0
000452631 245__ $$aStudying the nature of the unidentified gamma-ray source HESS J1841−055 with the MAGIC telescopes
000452631 260__ $$aOxford$$bOxford Univ. Press$$c2020
000452631 3367_ $$2DRIVER$$aarticle
000452631 3367_ $$2DataCite$$aOutput Types/Journal article
000452631 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1632992565_2518
000452631 3367_ $$2BibTeX$$aARTICLE
000452631 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000452631 3367_ $$00$$2EndNote$$aJournal Article
000452631 500__ $$a11 pages, 8 figures, 5 tables. Accepted in MNRAS
000452631 520__ $$aWe investigate the physical nature and origin of the gamma-ray emission from the extended source HESS J1841−055 observed at TeV and GeV energies. We observed HESS J1841−055 at TeV energies for a total effective time of 43 h with the MAGIC telescopes, in 2012 and 2013. Additionally, we analysed the GeV counterpart making use of about 10 yr of Fermi-LAT data. Using both Fermi-LAT and MAGIC, we study both the spectral and energy-dependent morphology of the source for almost four decades of energy. The origin of the gamma-ray emission from this region is investigated using multiwaveband information on sources present in this region, suggested to be associated with this unidentified gamma-ray source. We find that the extended emission at GeV–TeV energies is best described by more than one source model. We also perform the first energy-dependent analysis of the HESS J1841−055 region at GeV–TeV. We find that the emission at lower energies comes from a diffuse or extended component, while the major contribution of gamma rays above 1 TeV arises from the southern part of the source. Moreover, we find that a significant curvature is present in the combined observed spectrum of MAGIC and Fermi-LAT. The first multiwavelength spectral energy distribution of this unidentified source shows that the emission at GeV–TeV energies can be well explained with both leptonic and hadronic models. For the leptonic scenario, bremsstrahlung is the dominant emission compared to inverse Compton. On the other hand, for the hadronic model, gamma-ray resulting from the decay of neutral pions (π^0) can explain the observed spectrum. The presence of dense molecular clouds overlapping with HESS J1841−055 makes both bremsstrahlung and π^0-decay processes the dominant emission mechanisms for the source.
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000452631 588__ $$aDataset connected to CrossRef
000452631 650_7 $$2INSPIRE$$agamma ray: emission
000452631 650_7 $$2INSPIRE$$amodel: hadronic
000452631 650_7 $$2INSPIRE$$aHESS
000452631 650_7 $$2INSPIRE$$aMAGIC
000452631 650_7 $$2INSPIRE$$aGLAST
000452631 650_7 $$2INSPIRE$$aenergy dependence
000452631 650_7 $$2INSPIRE$$aenergy spectrum
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000452631 650_7 $$2INSPIRE$$abremsstrahlung
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000452631 650_7 $$2autogen$$aISM: individual objects: HESS J1841−055
000452631 650_7 $$2autogen$$aISM: supernova remnants
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000452631 650_7 $$2autogen$$aradiation mechanisms: non-thermal
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