Dark matter in the Milky Way, II. the HI gas distribution as a tracer of the gravitational potential
P.M.W. Kalberla, L. Dedes, J. Kerp, U. Haud

TL;DR
This study models the Milky Way's dark matter distribution using HI gas data, revealing a massive halo, a dark matter disk, and a ring, which together explain the galaxy's gravitational potential and structure.
Contribution
It provides the first detailed 3D HI density distribution out to 40 kpc, incorporating a self-consistent dark matter disk and ring, advancing understanding of galactic mass components.
Findings
Identification of a massive extended dark matter halo (~1.8×10^{12} Msun)
Detection of a dark matter disk (~2-3×10^{11} Msun)
Discovery of a dark matter ring at 13-18.5 kpc with M=2.2-2.8×10^{10} Msun
Abstract
Context. Gas within a galaxy is forced to establish pressure balance against gravitational forces. The shape of an unperturbed gaseous disk can be used to constrain dark matter models. Aims. We derive the 3-D HI volume density distribution for the Milky Way out to a galactocentric radius of 40 kpc and a height of 20 kpc to constrain the Galactic mass distribution. Methods. We used the Leiden/Argentine/Bonn all sky 21-cm line survey. The transformation from brightness temperatures to densities depends on the rotation curve. We explored several models, reflecting different dark matter distributions. Each of these models was set up to solve the combined Poisson-Boltzmann equation in a self-consistent way and optimized to reproduce the observed flaring. Results. Besides a massive extended halo of M ~ 1.8 10^{12} Msun, we find a self-gravitating dark matter disk with M=2 to 3 10^{11} Msun,…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
