Fig. 18.

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Frequency-averaged velocity level as a function of M⋆ measured above 125 μHz (circles,
) and below 30 μHz (diamonds,
) for the stars in our sample and for ℓ = 1 (left), ℓ = 2 (centre), and ℓ = 3 (right) modes. To avoid biases in the comparison, we do not consider
for stars with νc, 1 < 40 μHz. In each panel, the mean values of the
and
distributions are shown by the dashed and dotted lines, respectively. In each panel, the mean velocity levels computed with the VIRGO/SPM solar time series
are shown using the usual solar symbol, ⊙. The solar symbol enclosed by a square corresponds to
, while the other corresponds to
.
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