Fig. 27
Equivalent width measurements from October and December 2000 datasets for all the Y ii and Sr ii lines used in inversion and examples of Ti ii and Cr ii measurements. The values are from the first stellar rotation in October 2000 (plus) and last rotation in December 2000 (asterisk). The value is the mean of the observations obtained within one night. The error is the standard deviation of the measurements. The ordinates have different scales.
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