The results from 65 lunar occultation observations between August 1984 and July 1986 are discussed. The instrumentation and reduction procedures used in the study are described. Parameters are given for nine different double/multiple stars and for two stars with measurable angular diameters. Three newly discovered double stars, SAO 77310, SAO 79241, and the brighter component of SAO 77837, are examined. In addition, a fourth star, the brighter component of SAO 76862, is resolved for the first time.
No takes yet. Share an insight, caveat, or question.
Schmidtke et al. (1989) studied this question.