Variable stars in the Large Magellanic Cloud cluster NGC 1786

Details Variable stars in the Large Magellanic Cloud cluster NGC 1786 Variable stars in the Large Magellanic Cloud cluster NGC 1786

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..676g&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Aug. 1985, p. 676-680.

Other

5

Blue Stars, Giant Stars, Globular Clusters, Magellanic Clouds, Variable Stars, Astronomical Photography, Cepheid Variables, Milky Way Galaxy, Stellar Luminosity

Scientific paper

Twelve short-period variable stars have been identified in the Large Magellanic Cloud cluster NGC 1786. Periods have been obtained for ten stars. The period distribution is characteristic of a cluster of Oosterhoff type II. One variable is about a magnitude brighter than the others and may be a member of the class of anomalous Cepheids described by Zinn.

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