M–L relation of the Hyades open cluster. Black points with error bars show the position (mass, absolute V-magnitude) of 92 Hyades members whose common age (640 ± 7 Myr) and individual masses have been obtained by SPInS. The corresponding SPInS inferred isochrone is plotted in black. The positions of 17 stars, members of binary or triple systems and not included in the 92 star sample, are shown. Their dynamical masses have been inferred directly from observations and are therefore independent of stellar models.
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