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.
Title resolution pending
2 Pith papers cite this work, alongside 7 external citations. Polarity classification is still indexing.
2
Pith papers citing it
7
external citations · OpenAlex
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
U-Net inversion of red-clump extinction yields Galactic-plane dust density maps to 7 kpc with a 2.90 kpc exponential scale length and M74-like spiral morphology.
citing papers explorer
-
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.
-
A Face-on View of Interstellar Dust in the Galactic Plane
U-Net inversion of red-clump extinction yields Galactic-plane dust density maps to 7 kpc with a 2.90 kpc exponential scale length and M74-like spiral morphology.