4. CONCLUSIONS
V 1061 Tauri appears to be a very interesting system since there are relatively few systems known to share a common radiative envelope. Although there may be contamination by third light, the totality of primary minimum, if confirmed by higher-precision observations, would strengthen the light-curve solution. A radial-velocity study of this system would be very useful even if the system is only single lined because we have a well-determined photometric mass ratio in the case of a total eclipse. And, of course, if the system is double lined, that will only strengthen the determination of the mass ratio and the resulting fundamental quantities like the individual masses and radii. Further photoelectric observations in several passbands would also facilitate a simultaneous light and velocity solution. The solution presented here should be judged preliminary until further observations are made. We hope that observers will consider this potentially important system for their radial-velocity and light-curve observing programs.