The First Distance Constraint on the Renegade High Velocity Cloud
  Complex WD
  We present medium-resolution, near-ultraviolet VLT/FLAMES observations of the
star USNO-A0600-15865535. We adapt a standard method of stellar typing to our
measurement of the shape of the Balmer epsilon absorption line to demonstrates
that USNO-A0600-15865535 is a blue horizontal branch star, residing in the
lower stellar halo at a distance of 4.4 kpc from the Sun. We measure the H & K
lines of singly-ionized calcium and find two isolated velocity components, one
originating in the disk, and one associated with high-velocity cloud complex
WD. This detection demonstrated that complex WD is closer than ~4.4 kpc and is
the first distance constraint on the +100 km/s Galactic complex of clouds. We
find that Complex WD is not in corotation with the Galactic disk as has been
assumed for decades. We examine a number of scenarios, and find that the most
likely is that Complex WD was ejected from the solar neighborhood and is only a
few kpc from the Sun.
