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Fig. 5


Blue- and red- shifted emission of SO 1011−1010 at low velocities (| VVsys | < 1.9 km s-1, left panel) and in the higher velocity range where the emission is consistent with a rotating disk (HVdisk : 1.9 < | VVsys | < 3.5 km s-1, middle panel) is compared with C17O 3−2 emission in the HVdisk range (right panel, Codella et al. 2014a). The tilted black cross indicates the jet (PA = 22°) and the disk (PA = 112°) direction. The ellipse in the bottom left corner shows the beam HPBW of the line emission maps (, PA = 49°). First contour at 5σ with steps of 5σ for C17O 3−2 and at 3σ with steps of 1σ for SO 1011−1010.

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