Metal-rich giant branches of bulge clusters - Application to color-magnitude diagrams of M31 and M32

Details Metal-rich giant branches of bulge clusters - Application to color-magnitude diagrams of M31 and M32 Metal-rich giant branches of bulge clusters - Application to color-magnitude diagrams of M31 and M32

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...382l..15b&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 382, Nov. 20, 1991, p. L15-L17.

Astronomy and Astrophysics

Astronomy

58

Andromeda Galaxy, Color-Magnitude Diagram, Galactic Bulge, Metallicity, Abundance, Asymptotic Giant Branch Stars, Globular Clusters, Local Group (Astronomy), Star Distribution

Scientific paper

Metal-rich bulge globular clusters are compared with 47 Tuc in the M(Io) versus (V - I)o diagram. In addition to the expected red color shift and fading for increasing metallicity, the bulge clusters present a morphological change in the red giant branch which bends owing to blanketing effects. It is concluded that metal-rich population components similar to those of the star clusters NGC 6528 and NGC 6553 and Terzan 1 are below the observational cutoff.

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