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Fig. 12
Left: time evolution of the X-ray to bolometric luminosity ratio of a Sun-like star with different initial rotation periods on the ZAMS. Right: time evolution of the X-ray to bolometric luminosity ratio of main-sequence stars with masses in the range 0.4 ≤ M/M⊙ ≤ 1.2 for an initial rotation period P0 = 1.1 d on the ZAMS.
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