Photoelectric observations of lunar occultations.

A list of 8 photoelectric timings of lunar occultations is given. Five diameters have been measured and three double stars discovered. Thirteen recently determined diameters of late-type stars by interferometry and the lunar occultation method are used to show that only a small modification needs to be made to Wesselink's Vo-system surface brightness to (B-V)0 relationship.