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Fig. B.1

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Position–velocity diagram of the continuum subtracted C18O line along the disc major axis. The Δv is relative to the systemic velocity of 4.5 km s-1. The solid line shows the midplane Keplerian velocity for a stellar mass of 1 M and an inclination of 48°. The dashed lines correspond to stellar masses of 0.9 and 1.1 M. The data have been spectrally smoothed to a resolution of 80 m s-1. The spectro-spatial resolution is indicated in the lower left corner.

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