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Fig. 9
Distribution of the observed Q, S-complex and V-types asteroids in the BIC versus BAR space (only data with VNIR spectra are considered). The encircled regions are taken from Dunn et al. (2013) which follow the results of Gaffey et al. (1993); Burbine et al. (2001); Cloutis et al. (2010).
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