The Milky Way stellar disk shows a broken radial density profile with four components, azimuthal dependence, inner and outer flaring, and a density-metallicity bump possibly from radial migration.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Simulation of barred galaxy shows inside-out NSD growth and shared NSC history regulated by feedback, indicating bar timescale and cluster accretion are key to nuclear scaling relations and favoring lower Milky Way bulge mass.
citing papers explorer
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Mapping the Milky Way with Gaia Bp/Rp spectra-IV: the broken and asymmetric density profile of the stellar disk traced by a large sample of red clumps
The Milky Way stellar disk shows a broken radial density profile with four components, azimuthal dependence, inner and outer flaring, and a density-metallicity bump possibly from radial migration.
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SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk
Simulation of barred galaxy shows inside-out NSD growth and shared NSC history regulated by feedback, indicating bar timescale and cluster accretion are key to nuclear scaling relations and favoring lower Milky Way bulge mass.