Fig. B.3.
Measurements of log g for TWA stars with disks (this study, black dots) and without disk (Stelzer et al. 2013, gray diamonds), as a function of their Teff, both derived with ROTFIT. Empty symbols identify objects with disputed membership to the TWA in Gagné et al. (2017). PMS isochrones from Baraffe et al.’s (2015) model grid are overlaid as blue dotted lines for comparison purposes.
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