Abundances of RGB stars in NGC 6752
Abundances of O, Fe, Al, Mg, Na and Li determined from high-resolutionand high signal-to-noise spectra of 21 red giant branch (RGB) stars inthe globular cluster NGC 6752 are presented. We demonstrate that theStrömgren c1 index correlates extremely well with themeasured NH, CH and CN indices and that variations in c1 aredue to differences in UV NH band strengths. As shown by G
