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

Integral-field spectroscopy of the young high-mass star IRAS13481-6124