All Tables

Table 1: Broadband colors in stellar magnitudes for pure hydrogen atmospheres. Models are computed with nonideal EOS and Los Alamos (TOPS) opacities. Temperatures $T_{\rm eff}$ are given in thousands K and $\log g$ are in cgs units.
Table 2: Broadband colors in stellar magnitudes for pure hydrogen NLTE atmospheres (results of TLUSTY195). Units are the same as in Table 1.
Table 3: Model atmospheres of $T_{\rm eff}= 20~000$ K, and $\log g =8.0$ (cgs units), with pure hydrogen or pure iron composition.
Table 4: Broadband colors in stellar magnitudes for pure iron atmospheres. Models are computed with nonideal EOS and Los Alamos (TOPS) opacities. Units of $T_{\rm eff}$ and $\log g$ are the same as in Table 1.
Table 5: Broadband colors in stellar magnitudes for stratified hydrogen/iron models with nonideal EOS and Los Alamos (TOPS) opacities. Units of $T_{\rm eff}$ and $\log g$ are the same as in Table 1. Transition depth is located at $\tau =10^{-3}$ .
Table 6: List of iron core candidate stars selected from the data by Provencal et al. (1998). Procyon B has been excluded already from their data.