A study of the elements copper through uranium in Sirius A: Contributions from STIS and ground-based spectra
Charles R. Cowley, Thomas R. Ayres, Fiorella Castelli, Austin F., Gulliver, Richard Monier, and Glenn Wahlgren

TL;DR
This study comprehensively measures the elemental abundances from copper to uranium in Sirius A using space- and ground-based spectra to understand its chemical history and compare it with similar stars.
Contribution
It provides the most complete elemental abundance analysis of Sirius A to date, revealing its status as a hot Am star with moderate elemental enhancements.
Findings
Most element abundances are 10-100 times above solar.
No extreme abundance excesses typical of some chemically peculiar stars.
Supports classification of Sirius A as a hot Am star.
Abstract
We determine abundances or upper limits for all of the 55 stable elements from copper to uranium for the A1 Vm star Sirius. The purpose of the study is to assemble the most complete picture of elemental abundances with the hope of revealing the chemical history of the brightest star in the sky, apart from the Sun. We also explore the relationship of this hot metallic-line (Am) star to its cooler congeners, as well as the hotter, weakly- or non-magnetic mercury-manganese (HgMn) stars. Our primary observational material consists of {\em Hubble Space Telescope} () spectra taken with the Space Telescope Imaging Spectrograph (STIS) in the ASTRAL project. We have also used archival material from the %\citep/{ayr10}. satellite, and from the Goddard High-Resolution Spectrograph (GHRS), as well as ground-based spectra from Furenlid, Westin, Kurucz, Wahlgren, and their…
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