Variable stars in the globular cluster NGC 6284

Details Variable stars in the globular cluster NGC 6284 Variable stars in the globular cluster NGC 6284

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85.1604c&link_type=abstract

Astronomical Journal, vol. 85, Dec. 1980, p. 1604-1611. Research supported by the National Research Council of Canada.

Astronomy and Astrophysics

Astronomy

9

Astronomical Photography, Globular Clusters, Magnitude, Variable Stars, Cepheid Variables, Light Curve, Mira Variables, Schmidt Cameras

Scientific paper

Five new variables have been found in NGC 6284. Of 15 variables in and around the cluster, periods have been determined for 13. Nine of these are RR Lyrae variables, two are Population II Cepheids, and two are Mira variables. Four of the RR Lyrae stars and both Cepheids may be members. This cluster has the highest metallicity for a cluster with Population II Cepheids. A distance of 12.9 kpc has been determined for NGC 6284.

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