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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 10.

Results of the single-plane fit for RX J1713. (a) Maps of ΔN g(1) derived from Equation (6) and (b) ﹩{\widehat{N}}_{{\rm{g}}}(1)﹩ derived from Equation (2). The superposed contours in both panels (a) and (b) indicate excess counts of TeV gamma rays. The lowest contour level and contour intervals are 12 and 5 counts, respectively. (c) A plot of ΔN g(1) with respect to ﹩{\widehat{N}}_{{\rm{g}}}(1)﹩. The horizontal and vertical error bars shown in the left bottom corner indicate the median values of ﹩\sigma ({\widehat{N}}_{{\rm{g}}}(1))﹩ and σN g(1)) (see Equations (6) and (7) in Paper III), respectively.

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