Radial velocity observations obtained using digital reduction techniques are presented for a further six W Ursae Majoris-type contact binaries, namely TZ Boo, XY Boo, TX Cnc, RZ Com, CC Com and Y Sex. The derived spectroscopic mass ratios are found to be in good agreement with the photometric mass ratios determind by light curve synthesis techniques.
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McLean et al. (1983) studied this question.
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