Fig. 18
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Mass loss rates in M⊙ yr−1 as a function of solar luminosity. The ★-markers are the mass loss rates calculated from the models considered in this work, whereas the dot-dashed line using Krtička & Kubát (2017), and the dashed line is calculated using Björklund et al. (2021). The triangle markers are plotted from the empirical mass loss rate study by Hawcroft et al. (2021; their optically thick GA rates).
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