Search for high-mass protostars with ALMA revealed up to kilo-parsec scales (SPARKS) - I. Indication for a centrifugal barrier in the environment of a single high-mass envelope

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Fig. 13

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Left column: pv-diagram of models with a rotating ring with v_r ~ r (top panel), and with a disc in Keplerian rotation (bottom panel). Right column: colour scale showing the zeroth-moment maps for the 334.42 GHz CH₃OH v_t = 1 line (top panel) and the 346.456 GHz HC₃N v₇ = 1 line (bottom panel). Contours are the same as in the left column and show the model prediction.

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