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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.
citing papers explorer
-
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.
-
The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation
Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.