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.
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Observational proposal to obtain rest-frame optical stellar kinematics at z~2 with E-ELT to study bulge-disk continuum and co-evolution of mass, kinematics, and star formation.
citing papers explorer
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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.
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Morpho-kinematic of galaxies at cosmic noon
Observational proposal to obtain rest-frame optical stellar kinematics at z~2 with E-ELT to study bulge-disk continuum and co-evolution of mass, kinematics, and star formation.