Membership in the open cluster NGC 6494 - Astrometry with a PDS microdensitometer

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astrometry, Imaging Techniques, Open Clusters, Star Distribution, Microdensitometers, Milky Way Galaxy

Scientific paper

An image position finding procedure for PDS microdensitometer measures
of astrometric plates is described and applied to the open cluster NGC
6494. Probabilities of membership based on relative proper motions for
304 stars in the cluster field yield a cluster proper motion dispersion
(m.e.) of 0.0005 and 169 probable members.

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