Uvby-Beta Photometry of the Open Cluster M52

Details Uvby-Beta Photometry of the Open Cluster M52 Uvby-Beta Photometry of the Open Cluster M52

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pasp...93..447d&link_type=abstract

Publications of the Astronomical Society of the Pacific, Vol. 93, P. 447, 1981

Astronomy and Astrophysics

Astronomy

14

Scientific paper

Photometric uvbyβ observations of the open cluster M52 (NGC 7654) are used to determine the cluster's distance modulus (V0 - Mυ = 10.83 ± 0.24) and mean cluster reddening (E(B - V) = 0.57). The likelihood of cluster membership of the F7 Ib supergiant 60°2532 is verified on evolutionary grounds; its absolute magnitude is determined to be Mυ = -4.42 ± 0.46. The cluster M52 is shown to be similar in age to the Pleiades and the α Persei cluster.

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