  We report the results of our high resolution optical spectroscopic monitoring
campaign ($\lambda$ = 3800 -- 8800 A, R = 30000 -- 45000) of the new FU
Orionis-type object HBC 722. We observed HBC 722 with the BOES 1.8-m telescope
between 2010 November 26 and 2010 December 29 and FU Orionis itself on 2011
January 26. We detect a number of previously unreported high-resolution K I and
Ca II lines beyond 7500 A. We resolve the H$\alpha$ and Ca II line profiles
into three velocity components, which we attribute to both disk and outflow.
The increased accretion during outburst can heat the disk to produce the
relatively narrow absorption feature and launch outflows appearing as high
velocity blue and redshifted broad features.
