Table 2: Observed and reddening-corrected calculated photometric parameters of HD 137509.
  b-y $m_{\rm 1}$ $c_{\rm 1}$ $\Delta a$ U-B V-B G-B $B_{\rm 1}-B$ $B_{\rm 2}-B$ $V_{\rm 1}-B$ X Y Z
observations -0.095 0.183 0.411 0.066 0.761 1.136 2.294 0.811 1.566 1.836 0.762 0.076 -0.067
t12250g38, mag -0.054 0.142 0.640 0.057 0.995 1.088 2.265 0.838 1.574 1.801 1.026 0.122 -0.045
t12250g38, non -0.040 0.134 0.653 0.033 1.010 1.069 2.261 0.846 1.564 1.777 1.046 0.073 -0.028
t12750g40, mag -0.057 0.141 0.572 0.054 0.923 1.094 2.277 0.838 1.574 1.806 0.937 0.088 -0.044
t12750g40, non -0.044 0.135 0.586 0.031 0.941 1.075 2.271 0.846 1.565 1.783 0.957 0.045 -0.029
t13250g40, mag -0.059 0.135 0.516 0.051 0.860 1.105 2.293 0.834 1.578 1.815 0.863 0.077 -0.041
t13250g40, non -0.046 0.130 0.529 0.030 0.876 1.087 2.285 0.841 1.570 1.794 0.880 0.040 -0.028
t13750g42, mag -0.062 0.138 0.455 0.046 0.798 1.106 2.299 0.839 1.574 1.815 0.780 0.029 -0.040
t13750g42, non -0.051 0.138 0.468 0.030 0.815 1.081 2.282 0.850 1.561 1.788 0.790 -0.023 -0.030
t12750g38, mag -0.056 0.135 0.573 0.054 0.919 1.101 2.283 0.833 1.579 1.812 0.936 0.107 -0.043
t12750g38, non -0.043 0.129 0.588 0.032 0.936 1.082 2.277 0.841 1.570 1.790 0.957 0.066 -0.028
t12750g38, scaled -0.026 0.116 0.581 0.014 0.932 1.061 2.264 0.847 1.564 1.766 0.942 0.032 -0.016
$^\ast$t13750g42, mag -0.081 0.153 0.453 0.062 0.800 1.136 2.321 0.829 1.585 1.847 0.799 0.081 -0.051
$^\ast$t13750g42, non -0.064 0.144 0.470 0.037 0.820 1.111 2.307 0.837 1.576 1.819 0.818 0.040 -0.036
Theoretical colors were calculated for the models with (``mag'') and without (``non'') magnetic field, using individual abundances. Predictions for the scaled-solar abundance non-magnetic model are given for comparison. The last row reports predictions for the magnetic and non-magnetic models with revised abundances determined in the present paper.


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