Eta Carinae's gamma-ray emission is tied to hadronic acceleration in its colliding stellar winds, and CTA observations of its orbital variability could map the wind geometry and the injected proton and positron flux.
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Gamma-rays and positrons from Colliding Wind Binaries
Eta Carinae's gamma-ray emission is tied to hadronic acceleration in its colliding stellar winds, and CTA observations of its orbital variability could map the wind geometry and the injected proton and positron flux.