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Fig. 3


Observed mass-loss rates vs. wind velocities of M-type AGB stars (Olofsson et al. 2002; González Delgado et al. 2003, plus signs) and the corresponding properties for the dynamical models (filled circles). Top panel: dynamical properties of the models in set D. Middle and bottom panels: dynamical properties of the models in set P, color–coded according to p-value. Generally, within a set of models with same p (e.g. the dark green sequence with p = −0.75) the mass-loss rate increases with increasing condensation temperature. For a more detailed discussion on the dynamical properties of model set P, see Paper I.

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