Fig. 3.
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Analog of the HR diagram for the stellar sub-sets from Table A.1 (open squares for positive, and rhombi for negatives drift rates, respectively), Table A.2 (crosses), and Table A.3 (solid squares). The solid line depicts the main sequence, obtained using stellar models of fast rotators (Amard et al. 2019) with maximal surface gravity log(g).
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