Fig. 7
Right: X-ray to bolometric luminosity ratios of M 35 sample stars vs. Rossby numbers. Left: X-ray luminosities of M 35 sample stars vs. rotation periods. The thin black lines in both graphs represent models of X-ray activity evolution of 0.8 M⊙ stars with initial rotation periods on the ZAMS ranging from 0.12 to 3.4 days (see Sect. 5).
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