Color-magnitude diagrams for four rich clusters of the Large Magellanic Cloud

Details Color-magnitude diagrams for four rich clusters of the Large Magellanic Cloud Color-magnitude diagrams for four rich clusters of the Large Magellanic Cloud

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196..369f&link_type=abstract

Astrophysical Journal, vol. 196, Mar. 1, 1975, pt. 1, p. 369-371, 373, 375, 377-380.

Astronomy and Astrophysics

Astrophysics

30

Giant Stars, Globular Clusters, Magellanic Clouds, Stellar Evolution, Astronomical Photometry, Color, Photographic Plates, Star Distribution, Stellar Luminosity, Tables (Data)

Scientific paper

Color-magnitude diagrams are presented for four very rich clusters of the Large Magellanic Cloud. Comparisons with theoretical color-magnitude diagrams show good agreement in the location and distribution of stars in the giant regions. All four have nearly identical ages of approximately 50 million years. Each cluster has at least one anomalously luminous giant of intermediate color and magnitude of about -5.7, over a magnitude brighter than both the observed and predicted giant branch.

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