Fig. 11.
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Fractional radius, relative to the orbital separation, for primaries in Algols with and without disks. Red dots represents to the DPV stars. Below the circularization radius (shown by the solid bottom line), a disk should be formed, and below the top line, a disk might be formed. Semidetached Algol primaries from Dervişoǧlu et al. (2010) are also shown, as gray points. This figure is adapted from Mennickent et al. (2016a).
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