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.
Z $T_{\rm eff}$ $\log g$ U-B B-V V-R V-I
26 20 7 -1.330 -0.284 0.097 -0.063
26 20 8 -1.188 -0.191 0.011 -0.133
26 20 9 -1.110 -0.111 -0.047 -0.185
26 20 10 -1.094 -0.088 -0.040 -0.191
26 30 7 -1.432 -0.225 -0.083 -0.287
26 30 8 -1.432 -0.214 -0.108 -0.278
26 30 9 -1.418 -0.214 -0.137 -0.284
26 30 10 -1.377 -0.231 -0.139 -0.279
26 50 7 -1.360 -0.363 -0.177 -0.432
26 50 8 -1.376 -0.313 -0.194 -0.467
26 50 9 -1.431 -0.256 -0.202 -0.459
26 50 10 -1.440 -0.235 -0.188 -0.418
26 70 7 -1.322 -0.387 -0.174 -0.420
26 70 8 -1.311 -0.396 -0.188 -0.443
26 70 9 -1.303 -0.379 -0.193 -0.459
26 70 10 -1.313 -0.340 -0.197 -0.467
26 100 7 -1.323 -0.376 -0.168 -0.423
26 100 8 -1.315 -0.358 -0.133 -0.321
26 100 9 -1.327 -0.419 -0.187 -0.442
26 100 10 -1.321 -0.425 -0.195 -0.461


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