Fig. 10

Combination of the temperatures in one plot: from B − V corrected for interstellar extinction, from MK – > Teff, from obs1-obs26 (Sect. 2), and from some extra data (indicated by “X”(X1 − 4), cf. text). The temperatures derived from the B − V and MK data combine reasonably well. The temperatures for obs1-obs2, obs4-obs6 also seem to follow the combined data, and the values for obs7-obs26 extend the data. The difference from obs2 is relatively large. This forms step 5.
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