2002ApJ...576L..65M

In this Letter, we report on the detection of a new feature in the complex structure of the horizontal branch (HB) of the Galactic globular cluster NGC 6752. In the U versus (U-V)-plane, the HB shows a discontinuity (``jump'') at U-V≃-1.0 (corresponding T<sub>eff</sub>∼23,000 K). This ``second U-jump'' adds to the u-jump identified by F. Grundahl et al. in a dozen clusters at T_eff∼11,500 K. We show that this new discontinuity might be due to the combination of post-zero-age HB evolution and diffusion effects. We identify 11 asymptotic giant branch manqué stars. The comparison between post-HB star counts and evolutionary lifetimes, as predicted by canonical stellar models, shows good agreement, at variance with similar estimates for NGC 6752 available in the literature.