Investigating Non-LTE Abundances of Neodymium in Metal-poor FGK Stars

The dominant site(s) of the r-process are a subject of current debate. Ejecta from r-process-enrichment events like kilonovae are difficult to directly measure, so we must instead probe abundances in metal-poor stars to constrain r-process models. This requires state-of-the-art non-LTE (NLTE) modeli...

Ausführliche Beschreibung