Table 1
General comparison of the obtained signals showing the advantages of different molecules for various spectral type investigations.
Spectral type | Tphot/Tspot | Minimum residual intensity | Maximum Stokes V/Ic [%] | Maximum Stokes Q/Ic [%] | |||||||||
|
|||||||||||||
TiO | MgH | CaH | FeH | TiO | MgH | CaH | FeH | TiO | MgH | CaH | FeH | ||
|
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M | 3500 K/2800 K | 0.702 | 0.671 | 0.661 | 0.688 | 0.707 | 0.758 | 0.730 | 0.704 | 0.410 | 0.153 | 0.414 | 0.166 |
3500 K/3000 K | 0.705 | 0.667 | 0.660 | 0.692 | 0.988 | 1.016 | 1.078 | 0.829 | 0.529 | 0.218 | 0.599 | 0.199 | |
3800 K/3000 K | 0.800 | 0.690 | 0.771 | 0.723 | 0.659 | 0.602 | 0.712 | 0.623 | 0.352 | 0.125 | 0.395 | 0.150 | |
4000 K/3000 K | 0.866 | 0.701 | 0.830 | 0.741 | 0.498 | 0.404 | 0.535 | 0.513 | 0.266 | 0.084 | 0.297 | 0.123 | |
4000 K/3500 K | 0.860 | 0.692 | 0.829 | 0.746 | 1.086 | 1.058 | 1.436 | 0.877 | 0.491 | 0.226 | 0.616 | 0.222 | |
|
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K | 4200 K/3500 K | 0.919 | 0.715 | 0.884 | 0.774 | 0.833 | 0.724 | 1.096 | 0.729 | 0.376 | 0.155 | 0.470 | 0.184 |
4500 K/3500 K | 0.970 | 0.806 | 0.957 | 0.871 | 0.600 | 0.461 | 0.784 | 0.576 | 0.270 | 0.100 | 0.336 | 0.145 | |
4500 K/3800 K | 0.969 | 0.800 | 0.954 | 0.871 | 0.693 | 0.790 | 0.750 | 0.790 | 0.211 | 0.170 | 0.395 | 0.204 | |
4800 K/3800 K | 0.981 | 0.912 | 0.978 | 0.946 | 0.534 | 0.560 | 0.575 | 0.651 | 0.162 | 0.121 | 0.303 | 0.168 | |
4800 K/4000 K | 0.984 | 0.906 | 0.978 | 0.945 | 0.461 | 0.816 | 0.464 | 0.798 | 0.090 | 0.170 | 0.268 | 0.221 | |
5000 K/3800 K | 0.984 | 0.954 | 0.983 | 0.969 | 0.459 | 0.458 | 0.492 | 0.580 | 0.139 | 0.100 | 0.260 | 0.149 | |
5000 K/4000 K | 0.987 | 0.948 | 0.983 | 0.968 | 0.397 | 0.670 | 0.398 | 0.712 | 0.077 | 0.140 | 0.231 | 0.197 | |
5000 K/4200 K | 0.992 | 0.941 | 0.985 | 0.967 | 0.248 | 0.912 | 0.283 | 0.804 | 0.040 | 0.176 | 0.168 | 0.237 | |
|
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G | 5500 K/3800 K | 0.989 | 0.987 | 0.989 | 0.987 | 0.334 | 0.302 | 0.356 | 0.456 | 0.101 | 0.066 | 0.189 | 0.117 |
5500 K/4200 K | 0.994 | 0.978 | 0.990 | 0.985 | 0.182 | 0.608 | 0.206 | 0.634 | 0.030 | 0.118 | 0.123 | 0.187 | |
5500 K/4500 K | 0.999 | 0.977 | 0.996 | 0.989 | 0.035 | 0.580 | 0.085 | 0.471 | 0.010 | 0.182 | 0.041 | 0.149 | |
5800 K/3800 K | 0.990 | 0.992 | 0.991 | 0.989 | 0.285 | 0.245 | 0.302 | 0.403 | 0.086 | 0.054 | 0.161 | 0.104 | |
5800 K/4200 K | 0.995 | 0.984 | 0.991 | 0.987 | 0.156 | 0.494 | 0.175 | 0.562 | 0.026 | 0.096 | 0.105 | 0.166 | |
5800 K/4500 K | 0.999 | 0.983 | 0.997 | 0.992 | 0.030 | 0.473 | 0.073 | 0.419 | 0.009 | 0.148 | 0.034 | 0.133 | |
6000 K/3800 K | 0.991 | 0.993 | 0.991 | 0.990 | 0.258 | 0.215 | 0.273 | 0.374 | 0.077 | 0.048 | 0.145 | 0.096 | |
6000 K/4200 K | 0.995 | 0.986 | 0.992 | 0.989 | 0.141 | 0.435 | 0.159 | 0.522 | 0.023 | 0.085 | 0.095 | 0.154 | |
6000 K/4500 K | 0.999 | 0.986 | 0.997 | 0.992 | 0.028 | 0.418 | 0.067 | 0.389 | 0.008 | 0.130 | 0.031 | 0.123 | |
6000 K/4800 K | 1.000 | 0.992 | 0.999 | 0.997 | 0.003 | 0.208 | 0.017 | 0.174 | 0.002 | 0.081 | 0.008 | 0.057 |
Notes. Calculations were made with various combinations of underlying models for each spectral type. We list the minimum residual intensity (I), Stokes V, and Stokes Q signals from the different molecular lines for a model star with vsini = 10 km s-1 and 10% of the longitudinal or transverse magnetic field of 3 kG. Tabulated maxima exclude excursions due to atomic lines that overlap the relevant molecular band.
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