Chemical evolution of the metal poor Globular Cluster NGC 6809
arXiv:1811.12457 · doi:10.1093/mnras/sty3208
Abstract
We present the abundances analysis for a sample of 11 red giant branch stars in the metal-poor globular cluster NGC 6809 based on high-resolution spectra. Our main goals are to characterize its chemical composition and analyze this cluster's behavior associated with the Multiple Population (MPs) phenomenon. In our work we obtained the stellar parameters and chemical abundances of 24 elements (O, Na, Mg, Al, Si, Ca, Ti, V, Cr, Mn, Fe, Co, Sc, Ni, Cu, Zn, Y, Zr, Ba, La, Ce, Eu, Nd and Dy). We found a radial velocity of 174.7 3.2 km and a mean iron content of [Fe/H]=-2.01 0.02 in good agreement with other studies. Moreover, we found a large spread in the abundances of the light elements O, Na and Al confirming the presence of a Na-O anti-correlation a Na-Al correlation. The Mg-Al anti-correlation is also present in our cluster. The and iron-peak elements show good agreement with the halo field star trend. The heavy elements are dominated by the r-process.
arXiv comment13 pages, 11 figures, 3 tables, accepted for publication in MNRAS
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