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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 11.

Results of the two-plane fit for RX J1713. (a)–(d) Maps of ΔN g(2) (left panels) and ﹩{\widehat{N}}_{{\rm{g}}}(2)﹩ (right panels) for the pixel groups 1 (ΔN g(1) > 0, top panels) and 2 (ΔN g(1) ≤ 0, middle panels). The superposed contours in each panel are identical to those in Figure 10. (e) A plot of ΔN g(2) with respect to ﹩{\widehat{N}}_{{\rm{g}}}(2)﹩. The horizontal and vertical error bars shown in the left bottom corner indicate the median values of ﹩\sigma ({\widehat{N}}_{{\rm{g}}}(2))﹩ and σN g(2)), respectively. The red circles and error bars denote pixel group 1 and the blue ones pixel group 2.

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