Rubidium and lead abundances in giant stars of the globular clusters M4 and M5
David Yong (1), David L. Lambert (2), Diane B. Paulson (3), Bruce W., Carney (4) ((1) RSAA, Mt Stromlo Observatory, (2) Univ. of Texas, (3), NASA/GSFC, (4) Univ. of North Carolina)

TL;DR
This study measures Rb and Pb abundances in giant stars of globular clusters M4 and M5, revealing differences in s-process element enrichment and suggesting similar nucleosynthetic processes despite different initial compositions.
Contribution
It provides detailed neutron-capture element abundances in M4 and M5 giants, highlighting the differences in s-process enrichment and confirming the uniformity of abundance ratios within each cluster.
Findings
M4 shows higher Rb and Pb abundances than M5.
Abundance ratios are consistent among stars within each cluster.
The s-process element ratios are similar in both clusters, indicating similar nucleosynthetic origins.
Abstract
We present measurements of the neutron-capture elements Rb and Pb for bright giants in the globular clusters M4 and M5. The clusters are of similar metallicity ([Fe/H] = -1.2) but M4 is decidedly s-process enriched relative to M5: [Ba/Fe] = +0.6 for M4 but 0.0 for M5. The Rb and Pb abundances were derived by comparing synthetic spectra with high-resolution, high signal-to-noise ratio spectra obtained with MIKE on the Magellan telescope. Abundances of Y, Zr, La, and Eu were also obtained. In M4, the mean abundances from 12 giants are [Rb/Fe] = 0.39 +/- 0.02 (sigma = 0.07), [Rb/Zr] = 0.17 +/- 0.03 (sigma = 0.08), and [Pb/Fe] = 0.30 +/- 0.02 (sigma = 0.07). In M5, the mean abundances from two giants are [Rb/Fe] = 0.00 +/- 0.05 (sigma = 0.06), [Rb/Zr] = 0.08 +/- 0.08 (sigma = 0.11), and [Pb/Fe] = -0.35 +/- 0.02 (sigma = 0.04). Within the measurement uncertainties, the abundance ratios…
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