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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 12.

Fitted coefficient a vs. the SNR radius of RX J0852. The error bar associated with each data point represents the standard error. The red circles and error bars represent pixel group 1, and the orange and blue represent pixel groups 2 and 3, respectively. The median values of a are shown for two bins of the normalized radius, with the vertical error bars showing the interquartile range (in each bin, the upper quartile is the same as the median).

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