Author:
Lawler J. E.,Hartog E. A. Den,Labby Z. E.,Sneden C.,Cowan J. J.,Ivans I. I.
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
66 articles.
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1. The R-Process Alliance: 2MASS J22132050–5137385, the Star with the Highest-known r-process Enhancement at [Eu/Fe] = +2.45*;The Astrophysical Journal;2024-08-01
2. Comparative study of kilonova opacities for three elements of the sixth period (hafnium, osmium, and gold) from new atomic structure calculations in Hf I–IV, Os I–IV, and Au I–IV;Astronomy & Astrophysics;2024-06-25
3. Experimental atomic data of spectral lines – I. Cs, Ba, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu, Hf, Re, and Os in the 370–1000 nm interval;Monthly Notices of the Royal Astronomical Society;2023-10-24
4. Atomic clocks highly sensitive to the variation of the fine-structure constant based on Hf ii, Hf iv, and W vi ions;Physical Review A;2022-09-16
5. The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks*;The Astrophysical Journal;2022-09-01