Astronomy & Astrophysics

Table 1: Results of the analysis of TX UMa, $\beta$ Per and XZ Pup B and V light curves obtained by solving the inverse problem for the Roche model. Gravity-darkening exponent of the cooler secondary component ( $\beta _{\rm c}$ ) is a free parameter.
Table 2: Results of the analysis of TW And, TW Cas B and V light curves obtained by solving the inverse problem for the Roche model. Gravity-darkening exponent of the cooler secondary component ( $\beta _{\rm c}$ ) is a free parameter.
Table 3: The results of analysis of AI Dra Strömgren ybv light curves and UX Her B and V light curves obtained by solving the inverse problem for the Roche model. The gravity-darkening exponent of the cooler secondary component ( $\beta _{\rm c}$ ) is a free parameter.
Table 4: Simultaneous analysis of AW Cam B and V light curves obtained by solving the inverse problem for the Roche model with fixed and photometrically estimated mass ratios. The gravity-darkening exponent of the cooler secondary component ( $\beta _{\rm c}$ ) is a free parameter.