Mass ratios of Hyades binaries derived from color-magnitude positions are inconsistent with random orbital orientations, and a deconvolved re-analysis yields a bimodal distribution that depends on primary mass.
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The Bimodal Mass Ratio Distribution of the Hyades
Mass ratios of Hyades binaries derived from color-magnitude positions are inconsistent with random orbital orientations, and a deconvolved re-analysis yields a bimodal distribution that depends on primary mass.