The color-magnitude diagram of NGC 288

Details The color-magnitude diagram of NGC 288 The color-magnitude diagram of NGC 288

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26as...57...75b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 57, July 1984, p. 75-90.

Astronomy and Astrophysics

Astrophysics

38

Astronomical Catalogs, Color-Magnitude Diagram, Globular Clusters, Hertzsprung-Russell Diagram, Stellar Color, Stellar Magnitude, Stellar Spectrophotometry, Abundance, Chemical Composition, Main Sequence Stars, Metallicity, Stellar Evolution, Subgiant Stars

Scientific paper

The details of a BV photographic photometry of a rich sample of stars in the field of NGC 288, extending down to the main sequence, are presented. The observational data are reported and the reduction procedures used to obtain the color-magnitude diagram (CMD) are presented. Three important parameters derived from the CMD, the helium abundance, metal content, and heavy element spread, are discussed. Gaps on the main branches and peculiar aspects of the CMD are addressed.

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