Fig. 10
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Micro-turbulent velocity of the sample stars, separated by spectral luminosity (Gr. 1 to 4), and by SpT and LC as a function of Teff (same symbols and colours as in Fig. 3). Overplotted in gray are the adopted vmac data with solid and open circles representing LC V/IV and LC III/I objects, respectively. The mean value of the upper detectability limit to vmac averaged ’by eye’ and the corresponding
are also provided to guide the eye (horizontal solid and dashed lines, respectively). In the bottom panel the solid curved line indicates the vmac–Teff calibration provided by Gray (1984). For more information, see the text.
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