Observations of R-Process Stars in the Milky Way and Dwarf Galaxies

TL;DR

This paper reviews spectroscopic observations of r-process element signatures in metal-poor stars within the Milky Way and dwarf galaxies, discussing their implications for understanding the origins and astrophysical sites of the r-process.

Contribution

It provides a comprehensive overview of observational evidence, theoretical expectations, and chemical evolution models related to the r-process in different galactic environments.

Findings

Universal r-process pattern observed in some stars

Deviations from universality among light r-process elements

R-process enrichment depends on galaxy mass and star formation history

Abstract

This chapter presents an overview of the recent progress on spectroscopic observations of metal-poor stars with r-process element signatures found in the Milky Way's stellar halo and satellite dwarf galaxies. Major empirical lessons related to the origins of the r-process are discussed, including the universality of the observed r-process pattern and deviations from universality among the light r-process elements and actinides. Different astrophysical sites of the r-process based on theoretical expectations are presented, including common and rare supernovae and neutron star mergers. A major distinguishing factor between r-process sites is their delay time distribution. The best constraints on the detailed r-process pattern come from Galactic halo r-process stars, but these cannot provide information on the environment of the stars' birth gas clouds. Studying r-process enrichment within dwarf galaxies can remedy the situation despite the fact that high-resolution spectroscopic observations of individual stars in these systems are very difficult to obtain. A general overview of dwarf galaxy properties and chemical evolution expectations depending on their mass and star formation duration is provided. The r-process trends depend on the stellar mass and star formation durations of dwarf galaxies in a way that clearly shows that the r-process is rare, prolific, and has both prompt and delayed sources. This work complements ongoing theoretical heavy-element nucleosynthesis explorations and experimental measurements of the properties of r-process nuclei, such as with the Facility for Rare Isotope Beams.