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An 18-year Fermi-LAT stacking limit on GeV $γ$-ray emission from particle-accelerating colliding-wind binaries
The wind-collision regions of massive colliding-wind binaries (CWBs) accelerate relativistic particles, as shown by their non-thermal radio synchrotron and, in $η$ Car, hard X-ray emission. Whether CWBs emit GeV $γ$rays as a population is unknown: only $η$ Car is unambiguously detected by the Fermi
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