A one-zone model fitted to radio observations of WR 102's bubble predicts that protons accelerated at the wind shock dominate high-energy emission but produce an undetectable gamma-ray flux.
Caprioli \ and\ author A
4 Pith papers cite this work. Polarity classification is still indexing.
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2026 4representative citing papers
Hybrid simulations of the ion Weibel instability require a minimum grid resolution that scales with Alfvénic Mach number to correctly reproduce magnetic-field growth and saturation without introducing unphysical whistler modes.
citing papers explorer
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High-energy Processes in the Bubbles of Wolf-Rayet Stars: The case of WR 102
A one-zone model fitted to radio observations of WR 102's bubble predicts that protons accelerated at the wind shock dominate high-energy emission but produce an undetectable gamma-ray flux.
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Ion Weibel Instability in the hybrid framework: the optimal resolution
Hybrid simulations of the ion Weibel instability require a minimum grid resolution that scales with Alfvénic Mach number to correctly reproduce magnetic-field growth and saturation without introducing unphysical whistler modes.
- Transport of electrons in tangled magnetic fields
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