Kinematic measurements in the inner Milky Way show vertex deviation and anisotropy consistent with a nuclear bar oriented at approximately 60-75 degrees to the line of sight.
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4 Pith papers cite this work. Polarity classification is still indexing.
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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.
Kinematically selected red clump stars give A_K/E_{H-K} = 1.259 ± 0.074, A_H/A_K = 1.794 ± 0.046, and a Nuclear Bulge stellar mass of 12.2 ± 2.6 × 10^8 solar masses.
citing papers explorer
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Kinematic hints of a nuclear bar in the Milky Way
Kinematic measurements in the inner Milky Way show vertex deviation and anisotropy consistent with a nuclear bar oriented at approximately 60-75 degrees to the line of sight.
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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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Extinction law and stellar mass in the Nuclear Bulge from kinematically-selected red clump stars
Kinematically selected red clump stars give A_K/E_{H-K} = 1.259 ± 0.074, A_H/A_K = 1.794 ± 0.046, and a Nuclear Bulge stellar mass of 12.2 ± 2.6 × 10^8 solar masses.
- A spectroscopic map of the Galactic centre: Integrated light and dynamical modelling