# Sc and neutron-capture abundances in Galactic low- and high-alpha field   halo stars

**Authors:** C. K. Fishlock, D. Yong, A. I. Karakas, A. Alves-Brito, J. Melendez,, P. E. Nissen, C. Kobayashi, A. R. Casey

arXiv: 1701.02423 · 2017-01-18

## TL;DR

This study analyzes neutron-capture and iron-peak element abundances in 27 Galactic halo stars, revealing distinct chemical signatures between low- and high-alpha populations linked to different star formation histories.

## Contribution

It provides the first detailed comparison of neutron-capture element ratios in low- and high-alpha halo stars, constraining AGB star contributions and star formation rates.

## Key findings

- Low-alpha stars have lower [Sc/Fe], [Zr/Fe], [La/Zr], [Y/Eu], and [Ba/Eu] ratios.
- Low-alpha stars exhibit abundance patterns similar to dwarf spheroidal galaxies.
- Differences in chemical patterns are linked to star formation rates and AGB star contributions.

## Abstract

We determine relative abundance ratios for the neutron-capture elements Zr, La, Ce, Nd, and Eu for a sample of 27 Galactic dwarf stars with -1.5 < [Fe/H] <-0.8. We also measure the iron-peak element Sc. These stars separate into three populations (low- and high-alpha halo and thick-disc stars) based on the [alpha/Fe] abundance ratio and their kinematics as discovered by Nissen & Schuster. We find differences between the low- and high-alpha groups in the abundance ratios of [Sc/Fe], [Zr/Fe], [La/Zr], [Y/Eu], and [Ba/Eu] when including Y and Ba from Nissen & Schuster. For all ratios except [La/Zr], the low-alpha stars have a lower abundance compared to the high-alpha stars. The low-alpha stars display the same abundance patterns of high [Ba/Y] and low [Y/Eu] as observed in present-day dwarf spheroidal galaxies, although with smaller abundance differences, when compared to the high-alpha stars. These distinct chemical patterns have been attributed to differences in the star formation rate between the two populations and the contribution of low-metallicity, low-mass asymptotic giant branch (AGB) stars to the low-alpha population. By comparing the low-alpha population with AGB stellar models, we place constraints on the mass range of the AGB stars.

## Full text

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## Figures

16 figures with captions in the complete paper: https://tomesphere.com/paper/1701.02423/full.md

## References

64 references — full list in the complete paper: https://tomesphere.com/paper/1701.02423/full.md

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Source: https://tomesphere.com/paper/1701.02423