Fig. 2
Top panel: comparison between observations and modelling obtained by LIME using the structure and abundance profile from Keto et al. (2014; in red). The best fit model is shown in blue, using the same structure but an ad hoc abundance profile. Bottom panel: abundance profile from Keto et al. (2014) in red and best fit ad hoc abundance profile in blue as a function of the radial distance from the core in arcsec (top axis) and AU (bottom axis).
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