  We present radial velocity measurements for 70 high confidence, and 34
potential binary systems in fields containing the Perseus Molecular Cloud,
Pleiades, NGC 2264, and the Orion A star forming region. 18 of these systems
have been previously identified as binaries in the literature. Candidate
double-lined spectroscopic binaries (SB2s) are identified by analyzing the
cross-correlation functions (CCFs) computed during the reduction of each APOGEE
spectrum. We identify sources whose CCFs are well fit as the sum of two
Lorentzians as likely binaries, and provide an initial characterization of the
system based on the radial velocities indicated by that dual fit. For systems
observed over several epochs, we present mass ratios and systemic velocities;
for two systems with observations on eight or more epochs, and which meet our
criteria for robust orbital coverage, we derive initial orbital parameters. The
distribution of mass ratios for multi-epoch sources in our sample peaks at q=1,
but with a significant tail toward lower q values. Tables reporting radial
velocities, systemic velocities, and mass ratios are provided online. We
discuss future improvements to the radial velocity extraction method we employ,
as well as limitations imposed by the number of epochs currently available in
the APOGEE database. The Appendix contains brief notes from the literature on
each system in the sample, and more extensive notes for select sources of
interest.
