  The \textit{Spitzer} SAGE survey has allowed the identification and analysis
of significant samples of Young Stellar Object (YSO) candidates in the Large
Magellanic Cloud (LMC). However the angular resolution of \textit{Spitzer} is
relatively poor meaning that at the distance of the LMC, it is likely that many
of the \textit{Spitzer} YSO candidates in fact contain multiple components. We
present high resolution \textit{K}-band integral field spectroscopic
observations of the three most prominent massive YSO candidates in the N113
H\,{\sc ii} region using VLT/SINFONI. We have identified six \textit{K}-band
continuum sources within the three \textit{Spitzer} sources and we have mapped
the morphology and velocity fields of extended line emission around these
sources. Br$\gamma$, He\,{\sc i} and H$_2$ emission is found at the position of
all six \textit{K}-band sources; we discuss whether the emission is associated
with the continuum sources or whether it is ambient emission. H$_2$ emission
appears to be mostly ambient emission and no evidence of CO emission arising in
the discs of YSOs has been found. We have mapped the centroid velocities of
extended Br$\gamma$ emission and He {\sc i} emission and found evidence of two
expanding compact H\,{\sc ii} regions. One source shows compact and strong
H$_2$ emission suggestive of a molecular outflow. The diversity of
spectroscopic properties observed is interpreted in the context of a range of
evolutionary stages associated with massive star formation.
