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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 4.

Spatial distribution of (a) N g, (b) N x, and (c) N p for RX J1713 (identical to the H.E.S.S.18 (E > 2 TeV) ﹩4\buildrel{\,\prime}\over{.} 8﹩ resolution data set in Paper III). The white polygon in each panel indicates the region of interest for the present analysis. The red polygon in panel (c) outlines the region where the H I absorption is corrected (see Section 2.3 of Paper III).

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