activity
20102026
most citedHD 65949: Rosetta Stone or Red Herring

28 citations · 75 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Evidence for neutron capture in heavy-metal hot subdwarfs: Far-UV spectroscopy of EC22536-5304 and LSIV-14 116

M. Dorsch, C. S. Jeffery, J. Deprince +8

Most hot subdwarfs (sdO/B) are low-mass core-helium-burning stars formed through binary interaction. A subgroup of intermediate He-rich sdOBs shows extreme heavy-metal (Z>30) enric…

physics.atom-ph2025

Study of thorium in hypersonic gas jets: Ionization potentials of Th and Th

A. Claessens, F. Ivandikov, M. Brasseur +10

Laser ionization spectroscopy was performed on both neutral and singly ionized Th with the aim of identifying the nuclear-clock isomer in the singly charged ionic state of…

astro-ph.HE2024★ 8 cited

Kilonova ejecta opacity inferred from new large-scale HFR atomic calculations in all elements between Ca (Z = 20) and Lr (Z = 103)

Jérôme Deprince, Gururaj Wagle, Sirine Ben Nasr +7

In the context of kilonova (KN) modeling, the present work focusses on large-scale atomic data and opacity computations for all heavy elements from Ca to Lr, with a special effort…

astro-ph.SR2024★ 18 cited

3D NLTE modelling of Y and Eu. Centre-to-limb variation and solar abundances

N. Storm, P. S. Barklem, S. A. Yakovleva +6

Context. Abundances of s- and r-process elements in Sun-like stars constrain nucleosynthesis in extreme astrophysical events, such as compact binary mergers and explosions of highl…

astro-ph.SR2019★ 21 cited

First discovery of trans-iron elements in a DAO-type white dwarf (BD)

L. Löbling, M. A. Maney, T. Rauch +4

We have identified 484 lines of the trans-iron elements (TIEs) Zn, Ga, Ge, Se, Br, Kr, Sr, Zr, Mo, In, Te, I, Xe, and Ba, for the first time in the ultraviolet spectrum of a DAO-ty…

astro-ph.SR2010★ 28 cited

HD 65949: Rosetta Stone or Red Herring

C. R. Cowley, S. Hubrig, P. Palmeri +5

HD 65949 is a late B star with exceptionally strong Hg II at 3984[A], but it is not a typical HgMn star. The Re II spectrum is of extraordinary strength. Abundances, or upper limit…