Cited by 135Galaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studiesCosmology and Gravitation Theories

Broken degeneracies: the rotation curve and velocity anisotropy of the Milky Way halo

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Deason, A. J., Belokurov, V., Evans, N. W., An, J.·2012·Monthly Notices of the Royal Astronomical Society: Letters

Abstract

We use distant blue horizontal branch stars with Galactocentric distances 16 < r < 48 kpc as kinematic tracers of the Milky Way dark halo. We model the tracer density as an oblate, power law embedded within a spherical power-law potential. Using a distribution function method, we estimate the overall power-law potential and the velocity anisotropy of the halo tracers. We measure the slope of the potential to be γ∼ 0.4, and the overall mass within 50 kpc is ∼4 × 1011 M⊙. The tracer velocity anisotropy is radially biased with β∼ 0.5, which is in good agreement with local solar neighbourhood studies. Our results provide an accurate outer circular velocity profile for the Milky Way and suggest a relatively high-concentration dark matter halo (cvir∼ 20).

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Crossref · 10.1111/j.1745-3933.2012.01283.x

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  • Most studies that assume an NFW profile for the Galactic halo argue that the halo has a very high concentration, typically ∼14 or higher.

    “Such studies argue that the Galactic halo has a very high concentration, typically ∼ 14 or higher”

    From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Deason et al. 2012

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Research works printed but not linked: 2

  1. Binney J., Tremaine S., 2008, Galactic Dynamics, 2nd edn. Princeton Univ. Press, Princeton, NJ
  2. Newberg H. J., Yanny B., 2006, J. Phys. Conf. Ser., 47, 195

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Authors
Deason, A. J., Belokurov, V., Evans, N. W., & An, J.
Affiliations
  • 1Institute of Astronomy, Madingley Road, Cambridge CB3 0HA
  • Chinese Academy of Sciences (CN)
Venue
Monthly Notices of the Royal Astronomical Society: Letters
Published
2012-07-01
Volume
424
Issue
1
Pages
L44-L48
ISSN
  • 1745-3925 (ISSN-L)
  • 1745-3933
OpenAlex
W1853900401
Cited by
133
References
2
Citations by year
2026: 1 · 2025: 5 · 2024: 4 · 2023: 3 · 2022: 5 · 2021: 4 · 2020: 14 · 2019: 13 · 2018: 9 · 2017: 14 · 2016: 17 · 2015: 14 · 2014: 12 · 2013: 14 · 2012: 4
FWCI
7.71
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society Letters (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Durham Research Online (Durham University) (submittedVersion, cc-by)
  • arXiv (Cornell University)
Funders
Science and Technology Facilities Council (ST/H00243X/1, ST/F00723X/1, ST/J001538/1)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Keywords
Milky Way dark matter halo, rotation curves, velocity anisotropy, blue horizontal branch stars, kinematic tracers, power-law potential, halo concentration, circular velocity profiles, solar neighborhood

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