The Distance to the Draco Intermediate-Velocity Cloud

The understanding of the nature of intermediate- and high-velocity gas in the Milky Way is hampered by a paucity of distance estimates to individual clouds. A project has been started at the David Dunlap Observatory to address this lack of distance measures by observing early-type stars along the line of sight toward these clouds and searching for sodium doublet absorption at the clouds' systemic velocities. Distances to foreground stars (no absorption) and background stars (with absorption) are estimated from spectroscopic parallax, and thus the distance to the bracketed cloud is estimated. In this Letter, we present the first result from this ongoing project: a measurement of the distance to the Draco Cloud, which is the most studied of the intermediate-velocity clouds. The result presented here is the first distance bracket that tightly constrains the position of the Draco Cloud. We briefly describe our target selection and observing methodology and then demonstrate absorption at the velocity of the Draco Cloud for one star (TYC 4194 2188) and a lack of absorption for several other stars. We derive a distance bracket to the Draco Cloud of 463^{+ 192}₋₁₃₆ to 618^{+ 243}₋₁₇₄ pc.