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Fig. 1

image

Average Iline in the Ca II IRT line at 8500.35 Å against the Teff of the investigated stars. The error bars correspond to the standard deviations of the line indices of individual spectra of the respective stars. The red line is a linear fit for the inactive stars exceeding ICa IRT = 0.6 Å. The four active stars are highlighted by their names.

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