Fig. 21.
Same as Fig. 20 but for associations around CN-strong stars (method III). Here, MG was computed using the spectrophotometric distances of the CN-strong stars as outlined in Sect. 3.2. Orange and green circles show the associations with the Sgr stream and Gaia-Enceladus that obey the selection criteria of Paper I but were not considered when estimating the fraction N1P/Ntot.
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