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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 13.

(a) Integrated intensity map of H I for RX J0852. The integration range is from 20–40 km s−1. The superposed contours represent the X-rays, and the contour levels denote 2.0, 2.5, 4.0, 6.5, 10.0, 14.5, and 20.0 × 10−4 counts s−1 pixel−1. (b) P–V diagrams of H I. The integration range is 133.°37–133.°78 in the R.A. for the P–V diagram.

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