Fig. 20

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Median RV (〈VR〉) of FPR sources as a function of their galactic latitude. Red sources are C-star candidates. The solid lines indicate median values over bins of galactic latitude. The curves show the median value and standard deviation of 〈VR〉 in bins of galactic latitude (for C-stars these statistics are limited to galactic longitudes between 30° and 330°, excluding regions where they are scarce).
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