Table 2:
Observed and reddening-corrected calculated photometric parameters of HD 137509.
|
b-y |
 |
 |
 |
U-B |
V-B |
G-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 |
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 |
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.
|
Source LaTeX |
All tables |
In the text