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The Gamma-Ray Origin of RX J0852.0-4622 Quantifying the Hadronic and Leptonic Components: Further Evidence for the Cosmic-Ray Acceleration in Young Shell-type SNRs

  • Authors: Yasuo Fukui, Maki Aruga, Hidetoshi Sano, Takahiro Hayakawa, Tsuyoshi Inoue, Gavin Rowell, Sabrina Einecke, Kengo Tachihara

Yasuo Fukui et al 2024 The Astrophysical Journal 961 .

  • Provider: AAS Journals

Caption: Figure 14.

Maps of (a) TeV gamma-ray excess counts (E > 100 GeV) (H.E.S.S. Collaboration 2018c) and (b) X-ray counts (E = 2.0–5.7 keV) (Paper II). The superposed contours indicate the 12CO(J = 1–0) intensity at V LSR = 20–40 km s−1 whose contour levels are 2.5, 5.0, 7.5, 12.5, and 17.5 K km s−1. Some molecular clouds in the western part of the shell are indicated as A–E.

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