Fig. 6
Mass-loss rate as a function of pulsation period for the models with winds, plotted as black triangles compared to observations of various galactic C-rich targets from various sources. The plotted relations come from Vassiliadis & Wood (1993) (dashed line), Groenewegen et al. (1998, their Eq. (9), C-miras; solid line), and De Beck et al. (2010, fit on their page 21; dotted line).
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