All Tables

Table 1: Stellar properties of Cha H $\alpha$ objects.
Table 2: Physical parameters of BDs/VLMSs in Chamaeleon I derived from a comparison of synthetic GAIA-cond models and high-resolution UVES spectra using different line profile setups: (from left to right) effective temperature, surface gravity, lithium abundance and EW of lithium. The given results are for (i) a fit to the full range of free model parameters: $T_{{\rm eff}}$ , $\log(g)$ , $\log(\epsilon)$ , radial velocity and rotational velocity (first row of each observation) and (ii) for a fit with fixed effective temperature as determined by Comerón et al. (2000) (second row).
Table 3: Physical parameters of BDs/VLMSs in Chamaeleon I derived from a comparison of synthetic GAIA-cond models and high-resolution by Natta et al. (2004) using different line profile setups: (from left to right) effective temperature, surface gravity, lithium abundance and EW of lithium. The given results are for (i) a fit to the full range of free model parameters: $T_{{\rm eff}}$ , $\log(g)$ , $\log(\epsilon)$ , radial velocity and rotational velocity (first row of each observation) and (ii) for a fit with fixed effective temperature as determined by Comerón et al. (2000) (second row).