Fig. 9.
HR-diagram of the Corona-Australis region including different evolutionary models (PARSEC 1.2S, Siess et al. 2000, BT-Settl and Baraffe et al. 2015). The solid and dashed lines represent isochrones and tracks, respectively. The corresponding ages and masses are indicated in each panel for the various models. The stellar ages and masses are given in units of Myr and solar mass, respectively.
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