r-Process Abundance Signatures in Metal-Poor Halo Stars

Abundance observations indicate the presence of rapid-neutron capture (i.e., r-process) elements in old Galactic halo and globular cluster stars. Recent observations of the r-process-enriched star BD+17◦3248 include new abundance determinations for the neutron-capture elements Cd I (Z=48), Lu II (Z = 71) and Os II (Z = 76), the first detections of these elements in metal-poor r-process-enriched halo stars. Combining these and previous observations, we have now detected 32 n-capture elements in BD+17◦3248. This is the most of any metal-poor halo star to date. For the most r-process-rich (i.e. [Eu/Fe] ≃ 1) halo stars, such as CS 22892-052 and BD+17◦3248, abundance comparisons show that the heaviest stable n-capture elements (i.e., Ba and above, Z ≥ 56) are consistent with a scaled solar system r-process abundance distribution. The lighter n-capture element abundances in these stars, however, do not conform to the solar pattern. These comparisons, as well as recent observations of heavy elements in metal-poor globular clusters, suggest the possibility of multiple synthesis mechanisms for the n-capture elements. The heavy element abundance patterns in most metal-poor halo stars do not resemble that of CS 22892-052, but the presence of heavy elements such as Ba in nearly all metal-poor stars without s-process enrichment indicates that r-process enrichment in the early Galaxy is common. Electronic address: (1) [email protected] (2) [email protected] (3) [email protected] (4) [email protected]