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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 1.

Maps of (a) TeV gamma-ray excess counts (E > 100 GeV) (H.E.S.S. Collaboration 2018c), (b) X-ray counts (E = 2.0–5.7 keV) (Paper II), and (c) ISM proton column density (this work) toward RX J0852. The superposed white contours in panels (a)–(c) indicate excess counts of TeV gamma rays (the lowest level and intervals are 120 and 40 counts, respectively). The black contours in panel (c) indicate the 12CO(J = 1–0) intensity integrated into a velocity range of 20–40 km s−1 (the contour levels are 2.5, 5.0, 7.5, 12.5, and 17.5 K km s−1). The dashed–dotted circle outlines the PWN unrelated to the SNR (see the H.E.S.S. Collaboration 2018c).

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