Fig. 11
Predicted radial velocity trend in the direction of NGC 4463 from Galactic rotation, as a function of distance from the Sun (gray solid curve). The gray dotted lines show the 1σ extremes when uncertainties in the Galactic parameters are taken into account. The estimate derived for NGC 4463 is indicated by the full dot with error bars. The horizontal full and dotted lines show the RV of He 2-86 and its 1σ spread, respectively.
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