HSTPROMO Internal Proper-motion Kinematics of Dwarf Spheroidal Galaxies. I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco

van der Marel, Roeland P.; Watkins, Laura L.; Bellini, Andrea; Libralato, Mattia; Besla, Gurtina; Mamon, Gary A.; Sohn, Sangmo Tony; del Pino, Andrés; Pawlowski, Marcel S.; Vitral, Eduardo; Walker, Matthew G.

United States, France, Italy, Spain, Germany

Abstract

We analyze four epochs of Hubble Space Telescope imaging over 18 yr for the Draco dwarf spheroidal galaxy. We measure precise proper motions for hundreds of stars and combine these with existing line-of-sight (LOS) velocities. This provides the first radially resolved 3D velocity dispersion profiles for any dwarf galaxy. These constrain the intrinsic velocity anisotropy and resolve the mass–anisotropy degeneracy. We solve the Jeans equations in oblate axisymmetric geometry to infer the mass profile. We find the velocity dispersion to be radially anisotropic along the symmetry axis and tangentially anisotropic in the equatorial plane, with a globally averaged value βB¯=0.200.53+0.28 , (where 1 – βBvtan2/vrad2 in 3D). The logarithmic dark matter (DM) density slope over the observed radial range, Γdark, is 0.830.37+0.32 , consistent with the inner cusp predicted in

2024 The Astrophysical Journal
Gaia eHST 7