New LOFAR radio data and X-ray modeling indicate the extended source is thermal ICM emission from a massive merging galaxy cluster, unrelated to 1LHAASO J0343+5254u.
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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.
Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.
citing papers explorer
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Multi-wavelength insights into the pulsar wind nebula candidate near 1LHAASO J0343+5254u: an obscured merging galaxy cluster?
New LOFAR radio data and X-ray modeling indicate the extended source is thermal ICM emission from a massive merging galaxy cluster, unrelated to 1LHAASO J0343+5254u.
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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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The pulsar wind nebula around B1853+01 in X-rays
Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.