Abundances of Vanadium and Bromine in 3 Cen A: Additional Odd-Z Anomalies
C. R. Cowley, G. M. Wahlgren

TL;DR
This paper reports new abundance measurements of vanadium and bromine in the star 3 Cen A, supporting the diffusion theory for chemical peculiarities in such stars.
Contribution
It provides the first reported abundances of vanadium and bromine in 3 Cen A, adding evidence to the diffusion-based explanation of abundance anomalies.
Findings
Vanadium abundance excess of 1.2 dex
Bromine abundance excess of 2.6 dex
Supports diffusion as the cause of chemical peculiarities
Abstract
We report abundance excesses of 1.2 and 2.6 dex, respectively, for vanadium and bromine in the hot, peculiar star 3 Cen A. Abundances for these two odd-Z elements have not been previously reported for this star. Taken with previous work, they strengthen the case of the origin of the abundance peculiarities by diffusion.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astro and Planetary Science · Astrophysics and Star Formation Studies
