Dissecting the disk and the jet of a massive (proto)star - An ALMA view of IRAS 20126+4104

Open Access

Fig. 14

LSR velocity corresponding to the peak emission in the PV diagrams of the CH₃CN(12–11) K = 2, 3, 4, 5, 7, 8 lines as a function of the upper energy of the transition. The dashed line marks the systemic LSR velocity of −3.9 km s⁻¹.

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