V701 Sco
Bell1987 - Bell1987V (Johnson V)
The solution presented is essentially that of Bell & Malcolm (1987). They used the light curve model of Rucinksi (1976) and not the Wilson-Devinney model. The fillout factor was decreased from 0.63 to 0.58 to better fit their light curves using Binary Maker 3. The temperatures of both stars were held at 23500 K, as opposed to the model of Bell & Malcolm (1987) where they found one star to be 200 K cooler than the other. All other parameters were the same except for limb darkening. Bell & Malcolm used the limb darkening tables of Wade & Rucinski (1985) but do not give the values they used. The limb darkening values used here were taken from Van Hamme (1993).