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Paper detail

HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron

We present the detection of VHE gamma-ray emission above 100 TeV from HAWC J2227+610 with the HAWC observatory. Combining our observations with previously published results by VERITAS, we interpret the gamma-ray emission from HAWC J2227+610 as emission from protons with a lower limit in their cutoff energy of 800 TeV. The most likely source of the protons is the associated supernova remnant G106.3+2.7, making it a good candidate for a Galactic PeVatron. However, a purely leptonic origin of the observed emission cannot be excluded at this time.

preprint2020arXivOpen access
A. AlbertR. AlfaroC. AlvarezJ. R. Angeles CamachoJ. C. Arteaga-VelázquezK. P. ArunbabuD. Avila RojasH. A. Ayala SolaresV. BaghmanyanE. Belmont-MorenoS. Y. BenZviC. BrisboisK. S. Caballero-MoraT. CapistránA. CarramiñanaS. CasanovaU. CottiJ. CotzomiS. Coutiño de LeónE. de la FuenteL. Diaz-CruzB. L. DingusM. A. DuVernoisJ. C. Díaz-VélezR. W. EllsworthK. EngelC. EspinozaK. L. FanK. FangM. Fernández AlonsoH. FleischhackN. FraijaA. Galván-GámezD. GarciaJ. A. García-GonzálezF. GarfiasG. GiacintiM. M. GonzálezJ. A. GoodmanJ. P. HardingS. HernandezJ. HintonB. HonaD. HuangF. Hueyotl-ZahuantitlaP. HüntemeyerA. IriarteA. Jardin-BlicqV. JoshiW. H. LeeH. León VargasJ. T. LinnemannA. L. LonginottiG. Luis-RayaJ. LundeenK. MaloneS. S. MarinelliO. MartinezI. Martinez-CastellanosJ. Martínez-CastroJ. A. MatthewsP. Miranda-RomagnoliJ. A. Morales-SotoE. MorenoM. MostafáA. NayerhodaL. NellenM. NewboldM. U. NisaR. Noriega-PapaquiN. OmodeiA. PeiskerY. Pérez AraujoE. G. Pérez-PérezC. D. RhoD. Rosa-GonzálezE. Ruiz-VelascoH. SalazarF. Salesa GreusA. SandovalM. SchneiderH. SchoorlemmerJ. Serna FrancoG. SinnisA. J. SmithR. W. SpringerP. SurajbaliE. TabachnickM. TannerO. TibollaK. TollefsonI. TorresR. Torres-EscobedoF. Ureña-MenaL. VillaseñorT. WeisgarberA. ZepedaH. ZhouC. de LeónJ. D. Álvarez
astro-ph.HE
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A. AlbertR. AlfaroC. AlvarezJ. R. Angeles CamachoJ. C. Arteaga-VelázquezK. P. ArunbabuD. Avila RojasH. A. Ayala SolaresV. BaghmanyanE. Belmont-MorenoS. Y. BenZviC. BrisboisK. S. Caballero-MoraT. CapistránA. CarramiñanaS. CasanovaU. CottiJ. CotzomiS. Coutiño de LeónE. de la FuenteL. Diaz-CruzB. L. DingusM. A. DuVernoisJ. C. Díaz-VélezR. W. EllsworthK. EngelC. EspinozaK. L. FanK. FangM. Fernández AlonsoH. FleischhackN. FraijaA. Galván-GámezD. GarciaJ. A. García-GonzálezF. GarfiasG. GiacintiM. M. GonzálezJ. A. GoodmanJ. P. HardingS. HernandezJ. HintonB. HonaD. HuangF. Hueyotl-ZahuantitlaP. HüntemeyerA. IriarteA. Jardin-BlicqV. JoshiW. H. LeeH. León VargasJ. T. LinnemannA. L. LonginottiG. Luis-RayaJ. LundeenK. MaloneS. S. MarinelliO. MartinezI. Martinez-CastellanosJ. Martínez-CastroJ. A. MatthewsP. Miranda-RomagnoliJ. A. Morales-SotoE. MorenoM. MostafáA. NayerhodaL. NellenM. NewboldM. U. NisaR. Noriega-PapaquiN. OmodeiA. PeiskerY. Pérez AraujoE. G. Pérez-PérezC. D. RhoD. Rosa-GonzálezE. Ruiz-VelascoH. SalazarF. Salesa GreusA. SandovalM. SchneiderH. SchoorlemmerJ. Serna FrancoG. SinnisA. J. SmithR. W. SpringerP. SurajbaliE. TabachnickM. TannerO. TibollaK. TollefsonI. TorresR. Torres-EscobedoF. Ureña-MenaL. VillaseñorT. WeisgarberA. ZepedaH. ZhouC. de LeónJ. D. Álvarez

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