Monte Carlo population synthesis of young massive star clusters matches the combined H.E.S.S. Galactic Plane Survey and LHAASO first catalog for five parameter combinations, strongly disfavoring Bohm diffusion.
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LHAASO TeV sources associate with SNRs at 0.19, PWNe at 0.20, and microquasars at 0.027, with PWNe showing ~60% gamma-ray bright fraction and molecular clouds enhancing emission.
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Young Massive Star Clusters as TeV Emitters: Constraints from H.E.S.S. and LHAASO
Monte Carlo population synthesis of young massive star clusters matches the combined H.E.S.S. Galactic Plane Survey and LHAASO first catalog for five parameter combinations, strongly disfavoring Bohm diffusion.
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A Comparative Study of TeV Gamma-Ray Sources with Various Objects
LHAASO TeV sources associate with SNRs at 0.19, PWNe at 0.20, and microquasars at 0.027, with PWNe showing ~60% gamma-ray bright fraction and molecular clouds enhancing emission.