Photoelectric UBVRI Sequences in the Magellanic Cloud Clusters NGC 458, NGC 1783, and NGC 1841

Details Photoelectric UBVRI Sequences in the Magellanic Cloud Clusters NGC 458, NGC 1783, and NGC 1841 Photoelectric UBVRI Sequences in the Magellanic Cloud Clusters NGC 458, NGC 1783, and NGC 1841

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aj....110..646a&link_type=abstract

Astronomical Journal v.110, p.646

Astronomy and Astrophysics

Astronomy

14

Stars: Fundamental Parameters

Scientific paper

We present UBVRI photoelectric sequences for the Small Magellanic Cloud cluster NGC 458 and the Large Magellanic Cloud clusters, NGC 1783 and NGC 1841. All of them fall in fields suitable for CCD coverage. The number of stars and the range of magnitude and colors are NGC 458, 15 stars with 11.6 < V < 15.9, 0.0 < B - V < 1.2; NGC 1783, 10 stars with 13.1 < V < 15.9, -0.2 < B - V < 1.0; NGC 1841, 9 stars with 14.3 < V < 15.7, 0.6 < B - V < 1.2. The stars were measured an average of six times on at least three different nights. Four stars are in common with previous works in NGC 458 and four in NGC 1783.

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