Spectro-astrometry of the ESO-Hα 574 Hα emission in the UVES spectrum. Upper panel: UVES Hα line profile is shown and the narrow and broad components of the line are marked. Lower panel: Spectro-astrometric results are shown and the solid line is the analysis before continuum subtraction and the dashed line after continuum subtraction. The 1σ error is ~20 mas. The Hα line is offset in the outflow between ±140 km s^-1 and at least some of the broad component is found to be coincident with the stellar position.