A universal mass profile for dwarf spheroidal galaxies?

Matthew G. Walker, Mario Mateo, Edward W Olszewski, Jorge Penarrubia, N. Wyn Evans, Gerard Gilmore

Research output: Contribution to journalArticle

389 Citations (Scopus)

Abstract

We apply the Jeans equation to estimate masses for eight of the brightest dwarf spheroidal (dSph) galaxies. For Fornax, the dSph with the largest kinematic data set, we obtain a model-independent constraint on the maximum circular velocity, Vmax = 20+4 -3 km s-1. Although we obtain only lower limits of Vmax 10 km s-1 for the remaining dSphs, we find that in all cases the enclosed mass at the projected half-light radius is well constrained and robust to a wide range of halo models and velocity anisotropies. We derive a simple analytic formula that estimates M(rhalf ) accurately with respect to results from the full Jeans analysis. Applying this formula to the entire population of Local Group dSphs with published kinematic data, we demonstrate a correlation such that M(rhalf ) r1.4±0.4 half , or in terms of the mean density interior to the half-light radius, ρ r -1.6±0.4 half . This relation is driven by the fact that the dSph data exhibit a correlation between global velocity dispersion and half-light radius. We argue that tidal forces are unlikely to have introduced this relation, but tides may have increased the scatter and/or altered the slope. While the data are well described by mass profiles ranging over a factor of 2 in normalization (Vmax ∼ 10-20 km s-1), we consider the hypothesis that all dSphs are embedded within a "universal" dark matter halo. We show that in addition to the power law M ∞ r1.4, viable candidates include a cuspy "Navarro-Frenk-White" halo with Vmax ∼ 15 km s-1 and scale radius r0 ∼ 800 pc, as well as a cored halo with Vmax ∼ 13 km s-1 and r0 ∼ 150 pc. Finally, assuming that their measured velocity dispersions accurately reflect their masses, the smallest dSphs now allow us to resolve dSph densities at radii as small as a few tens of pc. At these small scales, we find mean densities as large as ρ 5 M pc-3 (200 GeV cm-3).

Original languageEnglish (US)
Pages (from-to)1274-1287
Number of pages14
JournalAstrophysical Journal
Volume704
Issue number2
DOIs
StatePublished - Oct 20 2009

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dwarf galaxies
halos
radii
profiles
kinematics
tides
estimates
power law
tide
anisotropy
dark matter
slopes

Keywords

  • Dwarf
  • Galaxies
  • Galaxies
  • Kinematics and dynamics
  • Local Group

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Walker, M. G., Mateo, M., Olszewski, E. W., Penarrubia, J., Evans, N. W., & Gilmore, G. (2009). A universal mass profile for dwarf spheroidal galaxies? Astrophysical Journal, 704(2), 1274-1287. https://doi.org/10.1088/0004-637X/704/2/1274

A universal mass profile for dwarf spheroidal galaxies? / Walker, Matthew G.; Mateo, Mario; Olszewski, Edward W; Penarrubia, Jorge; Evans, N. Wyn; Gilmore, Gerard.

In: Astrophysical Journal, Vol. 704, No. 2, 20.10.2009, p. 1274-1287.

Research output: Contribution to journalArticle

Walker, MG, Mateo, M, Olszewski, EW, Penarrubia, J, Evans, NW & Gilmore, G 2009, 'A universal mass profile for dwarf spheroidal galaxies?', Astrophysical Journal, vol. 704, no. 2, pp. 1274-1287. https://doi.org/10.1088/0004-637X/704/2/1274
Walker, Matthew G. ; Mateo, Mario ; Olszewski, Edward W ; Penarrubia, Jorge ; Evans, N. Wyn ; Gilmore, Gerard. / A universal mass profile for dwarf spheroidal galaxies?. In: Astrophysical Journal. 2009 ; Vol. 704, No. 2. pp. 1274-1287.
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