  We present results of AO-assisted K-band IFU spectroscopy of the massive
young star IRAS13481-6124 performed with ESO's VLT/SINFONI instrument. Our
spectro-astrometric analysis of the Br{\gamma} line revealed a photo-center
shift with respect to the adjacent continuum of \sim1 AU at a distance of 3.1
kpc. The position angle of this shift matches with that of the outflow which
confirms that the massive star is indeed the driving source. Furthermore, a
velocity gradient along the major disk axis was found which hints at the
rotational sense of the ionized region, and thus of the disk as well. The
gradient is not consistent with Keplerian motion but points to rigid rotation
of the innermost disk. Notably, emission of H_2 is absent from source while
both shocked and fluorescent H_2 emission are observed in its immediate
surroundings.
