RACE-OC project: rotation and variability in the ϵ Chamaeleontis, Octans, and Argus stellar associations

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Fig. 5

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The same as Fig. 4, but for Argus/IC 2391 association. The dashed and dotted lines represent mathematical functions describing the loci of the upper and lower bounds of the period distribution of α Persei members according to Barnes (2003).

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