Abstract:The systematic search for stellar multiplicity by observations of lunar occultations began in 1969. David Evans will review a large portion of the data collected since then in the second paper of this session. Here we will outline the historical development of the technique and comment on its limitations, contributions to double star research, and future improvements.Sir John Herschel (1865) may have been the first to suggest that “a double star, too close to be seen divided with any telescope, may yet be dete… Show more
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