Fig. 4
Comparison of the integrated ALMA intensities of H13CN(4−3) at radial offset points in the CSE of R Scl towards the west, east, north and south from the centre of the star with the best-fitting model which constrains the HCN molecular distributions at Re = 2 × 1015 cm. Error-bars on the observational points show 10% uncertainty on the flux calibration.
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