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Fig. 6

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Examples of different radial velocity distributions on the planetary disk and resulting velocity profiles, and the result from the retrieval. The example profiles assume a limb darkening coefficient of ϵ = 1. (a) Tidally locked rotation (according to WASP-189 b’s orbital period), (b) Day-to-night wind of vday–night = 5 km s−1. (c) Zonal jet with a speed of vjet = 5 km s−1 and a width of σjet = 0.3 Rp. (d) Velocity distributions according to the best-fitting parameters from the retrieval, and the average retrieved line profile calculated from 1000 random samples. The shaded region indicates the 1σ uncertainty interval.

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