Relative proper motions and membership assignments are presented for 526 stars located within a radius of 14arcmin of the center of M35 and extending to V ∼ 14.7. Ninety-nine of these stars were not included in Cudworth's (1971) study of this cluster. A vastly greater plate collection and longer epoch difference results in a three-fold increase in proper-motion precision over the earlier analysis. Three post-main-sequence stars are tentatively identified as belonging to the cluster. New photographic photometry casts doubt upon the claimed abundance anomalies within M35 reported by Vidal (1973).
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McNamara et al. (1986) studied this question.