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 $\tau =10^{-3}$.
Comp. $T_{\rm eff}$ $\log g$ U-B B-V V-R V-I
H/Fe 20 7 -1.300 -0.262 0.080 -0.057
H/Fe 20 8 -1.174 -0.180 -0.024 -0.141
H/Fe 20 9 -1.095 -0.097 -0.080 -0.192
H/Fe 20 10 -1.098 -0.091 -0.071 -0.197
H/Fe 30 7 -1.433 -0.216 -0.088 -0.287
H/Fe 30 8 -1.435 -0.207 -0.116 -0.282
H/Fe 30 9 -1.417 -0.209 -0.143 -0.288
H/Fe 30 10 -1.378 -0.229 -0.147 -0.285
H/Fe 50 7 -1.363 -0.357 -0.177 -0.429
H/Fe 50 8 -1.390 -0.299 -0.200 -0.466
H/Fe 50 9 -1.431 -0.255 -0.217 -0.451
H/Fe 50 10 -1.440 -0.235 -0.210 -0.415
H/Fe 70 7 -1.320 -0.381 -0.170 -0.413
H/Fe 70 8 -1.311 -0.390 -0.182 -0.425
H/Fe 70 9 -1.305 -0.374 -0.190 -0.445
H/Fe 70 10 -1.315 -0.338 -0.197 -0.461
H/Fe 100 7 -1.315 -0.364 -0.152 -0.376
H/Fe 100 8 -1.326 -0.392 -0.163 -0.382
H/Fe 100 9 -1.323 -0.408 -0.180 -0.428
H/Fe 100 10 -1.318 -0.419 -0.191 -0.452


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