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Cited article:

How many VHE gamma-ray binaries with young pulsars can be observed?

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Monte Carlo modeling of multi-PeV protons acceleration in gamma-ray binaries with strong stellar wind magnetic field

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Advances in Space Research (2026)
https://doi.org/10.1016/j.asr.2026.01.103

Galactic Superaccreting X-Ray Binaries as Super-PeVatron Accelerators

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PeV particle acceleration and nonthermal emission in the minimalist model of the extended jets in W50/SS433

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Physical Review D 112 (6) (2025)
https://doi.org/10.1103/wws6-3wz8

Particle acceleration and multi-messenger radiation from ultra-luminous X-ray sources

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Astronomy & Astrophysics 698 A188 (2025)
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An X-Ray Shell Reveals the Supernova Explosion for Galactic Microquasar SS 433

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The Astrophysical Journal Letters 975 (2) L28 (2024)
https://doi.org/10.3847/2041-8213/ad84ed

The Effect of Anisotropic Energy Injection on the Ejecta Emission

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The Astrophysical Journal 976 (1) 113 (2024)
https://doi.org/10.3847/1538-4357/ad81f4