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Cygnus X-3 as a semi-hidden PeVatron · DOI 10.1051/0004-6361/202554701

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astro-ph.HE 1

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2026 1

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UNVERDICTED 1

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Suppressed diffusion and gamma-ray emission from the Cygnus Bubble

astro-ph.HE · 2026-06-02 · unverdicted · novelty 4.0

Numerical transport modeling of the Cygnus Bubble finds that spatially dependent Bohm diffusion and strong suppression of the diffusion coefficient over at least 150 pc are required to match the observed gamma-ray spectrum and morphology, implying extreme assumptions for steady hadronic acceleration

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  • Suppressed diffusion and gamma-ray emission from the Cygnus Bubble astro-ph.HE · 2026-06-02 · unverdicted · none · ref 31

    Numerical transport modeling of the Cygnus Bubble finds that spatially dependent Bohm diffusion and strong suppression of the diffusion coefficient over at least 150 pc are required to match the observed gamma-ray spectrum and morphology, implying extreme assumptions for steady hadronic acceleration