Fig. 3.
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Macroturbulent velocity as a function of stellar parameters. From top left to bottom right: Θ versus v sin i, Θ versus Teff, Θ versus log g, and Θ versus log(ℒ/ℒ⊙). The marker size is proportional to ℒ, and the marker colour shows temperature Teff. The error bars in the lower right panel are only shown for our measurements as they are not available for the sample of Simón-Díaz et al. (2017).
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