Protostellar Outflows at the EarliesT Stages (POETS) VI. Evidence of disk-wind in G11.92-0.61 MM1

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Fig. 8

PV diagrams of CH₃CN υ = 0 J = 12−11 K = 3 (a), CH₃OH (b), SO₂ (c), and SO (d) emission for the cut at the position of the velocity spike (see the dotted black circle in Figs. 2k and 1). The magenta curves represent the Keplerian disk model for the central mass of 15 M_⊙.

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