Dynamical modelling of the Galactic bulge and bar: the Milky Way's bar
  pattern speed, stellar, and dark matter mass distribution
  We construct a large set of dynamical models of the galactic bulge, bar and
inner disk using the Made-to-Measure method. Our models are constrained to
match the red clump giant density from a combination of the VVV, UKIDSS and
2MASS infrared surveys together with stellar kinematics in the bulge from the
BRAVA and OGLE surveys, and in the entire bar region from the ARGOS survey. We
are able to recover the bar pattern speed and the stellar and dark matter mass
distributions in the bar region, thus recovering the entire galactic effective
potential. We find a bar pattern speed of $39.0 \pm 3.5
\,\rm{km\,s^{-1}\,kpc^{-1}}$, placing the bar corotation radius at $6.1 \pm 0.5
\rm{kpc}$ and making the Milky Way bar a typical fast rotator. We evaluate the
stellar mass of the long bar and bulge structure to be $M_{\rm{bar/bulge}} =
1.88 \pm 0.12 \times 10^{10} \, \rm{M}_{\odot}$, larger than the mass of disk
in the bar region, $M_{\rm{inner\ disk}} = 1.29\pm0.12 \times 10^{10} \,
\rm{M}_{\odot}$. The total dynamical mass in the bulge volume is
$1.85\pm0.05\times 10^{10} \, \rm{M}_{\odot}$. Thanks to more extended
kinematic data sets and recent measurement of the bulge IMF our models have a
low dark matter fraction in the bulge of $17\%\pm2\%$. We find a dark matter
density profile which flattens to a shallow cusp or core in the bulge region.
Finally, we find dynamical evidence for an extra central mass of
$\sim0.2\times10^{10} \,\rm{M}_{\odot}$, probably in a nuclear disk or disky
pseudobulge.
