Fig. 7.
Synthetic color-magnitude diagrams of bright globular cluster stars. All SCMDs were computed with the same input parameters; in particular, the same age, chemical composition, and number of stars. The location of the RGB tip is marked by a red horizontal line. For all the SCMDs, it is at MV = −2.15. The MV mag of the brightest stars are reported in each panel (VBS).
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