Open Access
Fig. 12.
Stellar filling factor, i.e., the ratio of the stellar radius to the Roche-lobe radius, as a function of the orbital phase (0 is mid-eclipse). Each colored stripe is obtained for a different set of extreme values observationally derived by Quaintrell et al. (2003), Rawls et al. (2011), and Falanga et al. (2015).
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