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Discovery of CO Clouds Associated with the X-Ray Jets of SS 433: Evidence for Shock–Cloud Interaction Enhancing Nonthermal X-Ray Emission

  • Authors: Haruka Sakemi, Hidetoshi Sano, Yasuo Fukui, Mami Machida, Shigeo S. Kimura, Masato I.N. Kobayashi, Kazuho Kayama, Hiroaki Yamamoto, Kengo Tachihara, Hiroshi Nagai

Haruka Sakemi et al 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

Caption: Figure 4.

Hardness ratio map between the 0.5–1.5 keV and 2.0–7.0 keV bands observed with XMM-Newton (K. Kayama et al. 2022, 2025). The images are regridded to match the spatial grid of the 12CO (J = 1–0) data, as in Figure 3. Magenta contours represent the CO integrated intensity over the same velocity ranges as in Figure 1. For the eastern side, three contour levels are shown from 2.1 to 3.5 K km s−1, while for the western side, six levels are shown from 0.8 to 2.0 K km s−1.

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