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 augmented with particle detectors is well suited to measure cosmic ray mass composition in the Galactic-extragalactic transition energy range, building on LOFAR experience.
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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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Origins of Cosmic Rays in the Galactic-extragalactic Transition Energy Range
SKA-Low augmented with particle detectors is well suited to measure cosmic ray mass composition in the Galactic-extragalactic transition energy range, building on LOFAR experience.