Upper panel: mean neutron-capture element abundance pattern for all “Ba-normal” (s-process deficient) stars in M 75. The solid line represents the best fit model for a scaled solar r-process plus 10% of the scaled solar s-process yields. The dashed line shows the scaled solar total r+s-process yields for comparison. The error bars represent the 1σ scatter of the derived element abundances of all s-process deficient stars; Bottom panel: derived n-capture elements abundances for star #901 – the most s-process rich star in our sample. The solid line represents the best fit model for a scaled solar total r+s-process yields. The dashed line shows the scaled solar pure r-process model for comparison. The error bars represent the random errors for this particular star.