Fig. 13
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 where the dust temperature is determined by radiative equilibrium (red squares) or set equal to the gas temperature (blue squares). The filled squares mark the dynamical models where a more detailed analysis is conducted.
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