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Hadronic Scenario for Galactic PeVatron LHAASO J1912+1014u Supported by Fermi-LAT γ-Ray Data and FUGIN CO Data

  • Authors: Tsunefumi Mizuno, Hidetoshi Sano, Takeru Murase, Tomohiko Oka, Hiromasa Suzuki, Naohito Nakahara

Tsunefumi Mizuno et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 6.

Relative contribution by each emission component (IC, eB, and pp) in the nominal case. Thin lines and thick lines show the results with Ecut,e = Ecut,p and Ecut,e = 30 TeV, respectively. The dashed and dotted vertical lines indicate the normalization energies of the fitted functions for WCDA and KM2A, as reported by Z. Cao et al. (2024).

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