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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SKAO's low- and mid-frequency arrays plus VLBI mode are projected to provide the sensitivity and sub-au resolution needed for systematic radio studies of Galactic wind-driven binaries.
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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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Enabling population studies on wind-driven Galactic binary systems
SKAO's low- and mid-frequency arrays plus VLBI mode are projected to provide the sensitivity and sub-au resolution needed for systematic radio studies of Galactic wind-driven binaries.