Cited by 104Stellar, planetary, and galactic studiesGalaxies: Formation, Evolution, PhenomenaCosmology and Gravitation Theories

The gravitational force field of the Galaxy measured from the kinematics of RR Lyrae in Gaia

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Wegg, Christopher, Gerhard, Ortwin, Bieth, Marie·2019·Monthly Notices of the Royal Astronomical Society

Abstract

From a sample of 15651 RR Lyrae with accurate proper motions in Gaia DR2, we measure the azimuthally averaged kinematics of the inner stellar halo between 1.5 and 20 kpc from the Galactic centre. We find that their kinematics are strongly radially anisotropic, and their velocity ellipsoid nearly spherically aligned over this volume. Only in the inner regions ${\lesssim } 5\, {\rm kpc}\,$ does the anisotropy significantly fall (but still with β > 0.25) and the velocity ellipsoid tilt towards cylindrical alignment. In the inner regions, our sample of halo stars rotates at up to $50\, {\rm km}\, {\rm s}^{-1}\,$, which may reflect the early history of the Milky Way, although there is also a significant angular momentum exchange with the Galactic bar at these radii. We subsequently apply the Jeans equations to these kinematic measurements in order to non-parametrically infer the azimuthally averaged gravitational acceleration field over this volume, and by removing the contribution from baryonic matter, measure the contribution from dark matter. We find that the gravitational potential of the dark matter is nearly spherical with average flattening $q_\Phi ={1.01 \pm 0.06\, }$ between 5 and 20 kpc, and by fitting parametric ellipsoidal density profiles to the acceleration field, we measure the flattening of the dark matter halo over these radii to be $q_\rho ={1.00 \pm 0.09\, }\!.$

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Research works printed but not linked: 3

  1. Bird S. A., Xue X.-X., Liu C., Shen J., Flynn C., Yang C., 2018, arXiv, 1805.04503 · arXiv
  2. Spergel D. N., Steinhardt P. J., 2000, Physical Review Letters, 84, 3760
  3. Watkins L. L., van der Marel R. P., Sohn S. T., Evans N. W., 2018, arXiv, 1804.11348 · arXiv

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Authors
Wegg, C., Gerhard, O., & Bieth, M.
Affiliations
  • Centre National de la Recherche Scientifique (FR)
  • Max Planck Institute for Extraterrestrial Physics (DE)
  • TNG Technology Consulting, Betastr. 13a, D-85774 Unterföhring, Germany
Corresponding author
Wegg, Christopher
Venue
Monthly Notices of the Royal Astronomical Society
Published
2019-02-26
Volume
485
Issue
3
Pages
3296-3316
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2952573599
Cited by
104
References
125
Citations by year
2026: 4 · 2025: 16 · 2024: 13 · 2023: 9 · 2022: 9 · 2021: 20 · 2020: 19 · 2019: 13 · 2018: 1
FWCI
8.18
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • HAL (submittedVersion, other-oa)
  • MPG.PuRe (Max Planck Society) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • European Union’s Horizon 2020 research (798384)
  • European Space Agency
  • National Aeronautics and Space Administration (NNX08AR22G)
  • National Science Foundation (AST-1238877)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Keywords
Milky Way gravitational potential, dark matter halos, RR Lyrae stars, Jeans equation, halo density profiles, halo flattening, galactic bars, angular momentum exchange

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