A proper-motion analysis of the cluster M35

Details A proper-motion analysis of the cluster M35 A proper-motion analysis of the cluster M35

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....91..557m&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 91, March 1986, p. 557-562.

Astronomy and Astrophysics

Astronomy

24

Astrometry, Star Clusters, Stellar Motions, Astronomical Photometry, Color-Magnitude Diagram, Histograms, Photographic Plates

Scientific paper

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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