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Fig. 4


Top panels: resulting radial profile of the DCO+ integrated intensity map of both models and data. The error bars on the data correspond to 3σ, where σ is calculated as the standard deviation of a single ellipsoid divided by the square root of the number of beams.Middle panels: models’ temperature profiles with contours at 19 and 30 K. Bottom panels: DCO+ abundance profiles over-plotted with temperature contours at 19 and 30 K. The hatched region in the DCO+ abundance from model CD marks the radial cutoff used in our standard model to reproduce the absence of emission at R > 300 AU.

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