Fig. 7.
Absolute magnitude of the Hyades white dwarfs as a function of the GBP − GRP colour. The error bars, smaller than the symbols, are always lower than 0.011 and 0.008 in absolute magnitude and GBP − GRP colour respectively. The WD cooling tracks of Bergeron et al. (2011) for various masses are shown in light blue (see text for more details).
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