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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 8.

Results of the three-plane fit for RX J0852. (a)–(f) Maps of ΔN g(3) (left panels) and ﹩{\widehat{N}}_{{\rm{g}}}(3)﹩ (right panels) for the pixel groups 1 (ΔN g(1) > 0.1, top panels), 2 (−0.1 ≤ ΔN g(1) ≤ 0.1, second row panels), and 3 (ΔN g(1) < − 0.1, third row panels). The superposed contours in each panel are identical to those in Figure 1. (g) A plot of ΔN g(3) with respect to ﹩{\widehat{N}}_{{\rm{g}}}(3)﹩. The horizontal and vertical error bars shown in the left bottom corner indicate the median values of ﹩\sigma ({\widehat{N}}_{{\rm{g}}}(3))﹩ and σN g(3)), respectively. The red circles and error bars denote pixel group 1, and the orange and blue ones denote pixel groups 2 and 3, respectively.

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