and comparison with the giants 24 Mar 2009 Barium isotopic ratios in metal-poor stars: calibrating the method with globular clusters 19 Aug 2025 Show more Show less Predictions from $s$-process AGB models of the isotopic variations of zirconium and neodym

 

and comparison with the giants 24 Mar 2009 Barium isotopic ratios in metal-poor stars: calibrating the method with globular clusters 19 Aug 2025 Show more Show less Predictions from $s$-process AGB models of the isotopic variations of zirconium and neodymium for comparison to bulk meteorites 28 Nov 2025 A coherent view of Li depletion and angular momentum transport to explain the Li plateau -- from Population II to Population I stars 22 Mar 2024 Atmospheric parameters and chemical abundances of the A-type eclipsing binary system RR Lyncis A and B 24 Sept 2025 MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars 18 Jan 2025 Spectroscopic study of the late B-type eclipsing binary system AR Aurigae A and B: Towards clarifying the differences in atmospheric parameters and chemical abundances 14 Jan 2025 Chemical Evolution of Ytterbium in the Galactic Disk 01 Feb 2022 Abundance of strontium in the Galactic globular cluster 47 Tuc 08 Oct 2025 , url ={ https://arxiv.org/abs/0910.1085 }, primaryClass ={ astro-ph.SR }。

year ={ 2009 }, eprint ={ 0910.1085 }, author ={ C. C. Worley and P. L. Cottrell and K. C. Freeman and E. C. Wylie-de Boer }, doi ={ https://doi.org/10.1111/j.1365-2966.2009.15520.x }, } AI detection Analyze Related papers A critical evaluation of the elemental abundances and evolutionary status of 15 Vul (HD 189849): The first identification of an evolved Am star 13 Jan 2025 First stars XII. Abundances in extremely metal-poor turnoff stars。

Copy @misc {worley2009differentialchemicalabundanceanalysis, title ={ Differential chemical abundance analysis of a 47 Tuc AGB star with respect to Arcturus }, archivePrefix ={ arXiv },。