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

We report the first identification of molecular clumps directly associated with the rebrightening regions of the large-scale X-ray jets of SS 433, based on ^12 CO ( J = 1–0) observations with the Nobeyama 45 m Radio Telescope. Multiple clumps are detected toward the eastern and western jet heads, sh...

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Hlavní autoři:	Haruka Sakemi, Hidetoshi Sano, Yasuo Fukui, Mami Machida, Shigeo S. Kimura, Masato I.N. Kobayashi, Kazuho Kayama, Hiroaki Yamamoto, Kengo Tachihara, Hiroshi Nagai
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2026-01-01
Edice:	The Astrophysical Journal Letters
Témata:	Stellar mass black holes X-ray binary stars Non-thermal radiation sources Molecular clouds
On-line přístup:	https://doi.org/10.3847/2041-8213/ae736b
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