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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 2.

Spatial distribution of (a) N g, (b) N x, and (c) N p for RX J0852. The three data sets are pixelated on an ﹩11\buildrel{\,\prime}\over{.} 4﹩ grid to match the H.E.S.S. resolution. The white polygon in each panel indicates the region of interest for the present analysis, and the dashed circle outlines the PWN unrelated to the SNR.

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