  We present the results of high-resolution (R $\ge$ 30,000) optical and
near-infrared spectroscopic monitoring observations of a FU Orionis-type
object, V960 Mon, which underwent an outburst in 2014 November. We have
monitored this object with the Bohyunsan Optical Echelle Spectrograph (BOES)
and the Immersion GRating INfrared Spectrograph (IGRINS) since 2014 December.
Various features produced by a wind, disk, and outflow/jet were detected. The
wind features varied over time and continually weakened after the outburst. We
detected double-peaked line profiles in the optical and near-infrared, and the
line widths tend to decrease with increasing wavelength, indicative of
Keplerian disk rotation. The disk features in the optical and near-infrared
spectra fit well with G-type and K-type stellar spectra convolved with a kernel
to account for the maximum projected disk rotation velocity of about
40.3$\pm$3.8 km s$^{-1}$ and 36.3$\pm$3.9 km s$^{-1}$, respectively. We also
report the detection of [S II] and H$_{2}$ emission lines, which are
jet/outflow tracers and rarely found in FUors.
