Membership of the Alpha Per cluster as determined by proper motion

Details Membership of the Alpha Per cluster as determined by proper motion Membership of the Alpha Per cluster as determined by proper motion

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85...66f&link_type=abstract

Astronomical Journal, vol. 85, Jan. 1980, p. 66-70.

Astronomy and Astrophysics

Astronomy

15

Astrometry, Star Clusters, Star Distribution, Stellar Motions, Data Correlation, Histograms, Statistical Distributions, Stellar Magnitude

Scientific paper

Probable member stars of the α Per cluster have been checked by Palomar Schmidt astrometric observations in a range of magnitude 7 to 12 and in an area of 5° × 5°. The membership of stars already assigned to the cluster on the basis of their proper motions is confirmed mainly for stars brighter than visual magnitude 11. This result is not contradictory with modern astrographic observations.

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