Fig. 7
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Phase-polarisation data in V for the asteroids currently named ‘Barbarians’, including the prototype of this class, asteroid (234) Barbara. Small members of the dynamical families of (729) Watsonia and (606) Brangane (see text) are not included in this figure, nor are a couple of measurements of (2085) Henan, another Barbarian candidate for which more data are needed. The meanings of the symbols are the same as in Fig. 1.
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