Multi-wavelength MCMC modeling of RCW 38 supports hadronic gamma-ray production with K_ep ≲ 10^{-3} and acceleration efficiency ≳1%, consistent with cosmic-ray composition requirements.
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SKA-Low is projected to reconstruct cosmic-ray air-shower depth of maximum with better than 8 g/cm² resolution and enable full reconstruction down to PeV energies via radio detection.
citing papers explorer
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A broadband view of the thermal and non-thermal emission from the embedded massive star cluster RCW 38
Multi-wavelength MCMC modeling of RCW 38 supports hadronic gamma-ray production with K_ep ≲ 10^{-3} and acceleration efficiency ≳1%, consistent with cosmic-ray composition requirements.
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Measuring High-Energy Cosmic Particles with the SKA
SKA-Low is projected to reconstruct cosmic-ray air-shower depth of maximum with better than 8 g/cm² resolution and enable full reconstruction down to PeV energies via radio detection.