A correct algorithm for the proper motion of cluster members

Details A correct algorithm for the proper motion of cluster members A correct algorithm for the proper motion of cluster members

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cha%26a..10..313z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 10, Issue 4, p. 313-317.

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper we give, for the case where the proper motions of stars are unknown, a method of calculating the correct relative proper motion, the linear model being assumed always. We also show that the proper motion usually found on assuming Σxμx = Σyμx = 0, Σxμy = Σyy = 0, Σμx = 0, Σμy = 0, is not the relative proper motion, and that the difference between the two depends on the positions of the reference stars on the plate.

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