Photoelectric UBVRI Sequences in the Magellanic Cloud Clusters NGC 152, NGC 1978, and NGC 2121

Details Photoelectric UBVRI Sequences in the Magellanic Cloud Clusters NGC 152, NGC 1978, and NGC 2121 Photoelectric UBVRI Sequences in the Magellanic Cloud Clusters NGC 152, NGC 1978, and NGC 2121

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....105.2118a&link_type=abstract

Astronomical Journal v.105, p.2118

Astronomy and Astrophysics

Astronomy

3

Magellanic Clouds, Globular Clusters: General

Scientific paper

We present UBVRI photoelectric sequences for the Small Magellanic Cloud blue cluster NGC 152 and the Large Magellanic Cloud red clusters NGC 1978 and NGC 2121. All of them fall in fields suitable for CCD coverage. The number of stars and the range of magnitude and colors are: NGC 152, eight stars with 12.7 < V < 16.1; 0.6 < B-V < 1.6; NGC 1978, ten stars with 13.1 < V < 15.3; -0.2< B-V < 1.7; NGC 2121, nine stars with 12.7 < V < 15.5; 0.5 < B-V < 1.2. The stars were measured an average of five times on at least three different nights. Six stars are in common with previous works in NGC 152, and two each in NGC 1978 and NGC 2121.

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