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Fig. 18.


Luminosity functions for NGC 3532 and the Pleiades. For NGC 3532 we show the empirical luminosity function (solid line) based on our radial velocity observations and an estimate for the inner 1° of the cluster (dashed line) based on the photometric membership. The Pleiades luminosity function (dotted line) is based on Bouy et al. (2015).

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