Abundances of field & GC RR Lyrae. I. NGC3201

We collected optical (4580-5330{AA}), high-resolution (~34000), high signal-to-noise ratio (~200) spectra for 11 RR Lyrae stars and one red horizontal branch star with the multifiber spectrograph M2FS with the 6.5m Magellan telescope at the Las Campanas Observatory. From measured equivalent widths, we derived atmospheric parameters and abundance ratios for {alpha} (Mg, Ca and Ti), iron-peak (Sc, Cr, Ni and Zn), and s-process (Y) elements.

We found that NGC 3201 is a homogeneous, monometallic ([Fe/H]=-1.47+/-0.04), {alpha}-enhanced ([{alpha}/Fe]=0.37+/-0.04) cluster. The relative abundances of the iron-peak and s-process elements were found to be consistent with solar values. In comparison with other large stellar samples, NGC 3201 RR Lyraes have similar chemical enrichment histories as do those of other old (t>=10Gyr) Halo components (globular clusters; red giants; blue and red horizontal branch stars; and RR Lyraes).