Photometric zero-point stars in Magellanic cloud clusters

Details Photometric zero-point stars in Magellanic cloud clusters Photometric zero-point stars in Magellanic cloud clusters

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99..179w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, March 1987, p. 179-182. NSF-supported research.

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12

Astronomical Photometry, Faint Objects, Magellanic Clouds, Star Clusters, Stellar Spectrophotometry, Ubv Spectra

Scientific paper

Photoelectric UBV measurements of faint stars in the Magellanic Cloud clusters NGC 339, NGC 458, NGC 2004, and NGC 2164, obtained with the 1.5-m Cerro Tololo Inter-American Observatory in 1972 and 1973, are presented. The present as-yet unpublished sample of stars range in V brightness from 15.2 to 18.0, and in (B-V) color from -0.20 to + 1.82. The data provide zero-point standards for use both in these clusters and in other clusters in the Magellanic Clouds.

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