articleThe Astrophysical JournalOct 1, 2009Closed access

A UNIVERSAL MASS PROFILE FOR DWARF SPHEROIDAL GALAXIES?

University of Cambridge · Institute of Astronomy · +2 more institutions

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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…

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Authors

6

Topics & keywords

Keywords
  • Physics
  • Astrophysics
  • Galaxy
  • Velocity dispersion
  • Halo
  • Dark matter
  • Local Group
  • Dwarf spheroidal galaxy
UN Sustainable Development Goals
  • Life below water
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