Fig. 12
The mass as a function of Teff for substellar objects, according to evolutionary models of 1 Myr and 5 Myr objects (Chabrier et al. 2000). The range of effective temperatures for CT Cha B from the best fit models is shown with solid lines and the range previously reported (Schmidt et al. 2008) is shown with dashed lines for comparison. The age of CT Cha B is expected to be between 1 Myr and 5 Myr.
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