Exoplanets & Stellar Populations Group

NGC 6752 has been largely studied in the past. It has a very well defined EBHB. Penny & Dickens (1986) have shown a B,V CCD study from a combination of data from two telescopes, and published a CMD from the RGB tip to V ~ 24 mag, though with a small number of measured stars. In the same year, Buonanno et al. (1986) show a CMD in the same bands for stars from ~1 mag above the TO to ~5 mag below it. More recently, Renzini et al. (1996) and Rubenstein & Baylin (1997) published a CMD from HST data.