Hadronic interactions cannot fully account for UHE gamma-ray emission from the six LHAASO microquasars; their contribution to the Galactic CR spectrum at 1 PeV is at most ~4% under baseline assumptions of 0.1 Myr injection and 10% efficiency.
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Constraints on Hadronic Emission from Microquasars Detected by LHAASO
Hadronic interactions cannot fully account for UHE gamma-ray emission from the six LHAASO microquasars; their contribution to the Galactic CR spectrum at 1 PeV is at most ~4% under baseline assumptions of 0.1 Myr injection and 10% efficiency.