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Revisiting inelastic Cu + H collisions and the non-LTE Galactic evolution of copper
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Early r-process Enrichment and Hierarchical Assembly Across the Sagittarius Dwarf Galaxy*
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Ariel stellar characterisation
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A conclusive non-detection of magnetic field in the Am star o Peg with high-precision near-infrared spectroscopy
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The Rise of the r-process in the Gaia-Sausage/Enceladus Dwarf Galaxy
∗
Xiaowei 筱葳 Ou 欧, Alexander P. Ji, Anna Frebel, Rohan P. Naidu and Guilherme Limberg The Astrophysical Journal 974(2) 232 (2024) https://doi.org/10.3847/1538-4357/ad6f9b
Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II*
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Surface distribution of small-scale magnetic field on the active cool star LQ Hydrae
Observational constraints on the origin of the elements – VII. NLTE analysis of Y ii lines in spectra of cool stars and implications for Y as a Galactic chemical clock
A cool, magnetic white dwarf accreting planetary debris
Stéphane Vennes, Adela Kawka, Beth L Klein, B Zuckerman, Alycia J Weinberger and Carl Melis Monthly Notices of the Royal Astronomical Society 527(2) 3122 (2023) https://doi.org/10.1093/mnras/stad3370
Observational constraints on the origin of the elements
Estimating fundamental parameters of nearby M dwarfs from SPIRou spectra
P I Cristofari, J-F Donati, T Masseron, et al. Monthly Notices of the Royal Astronomical Society 511(2) 1893 (2022) https://doi.org/10.1093/mnras/stab3679
Non-LTE abundance corrections for late-type stars from 2000 Å to 3 µm
Evidence from Disrupted Halo Dwarfs that r-process Enrichment via Neutron Star Mergers is Delayed by ≳500 Myr
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Comparative high-resolution spectroscopy of M dwarfs: Exploring non-LTE effects
I Negueruela, A-N Chené, H M Tabernero, et al. Monthly Notices of the Royal Astronomical Society 505(2) 1618 (2021) https://doi.org/10.1093/mnras/stab1117
Chemical diversity among A–B stars with low rotational velocities: non-LTE abundance analysis
L Mashonkina, T Ryabchikova, S Alexeeva, T Sitnova and O Zatsarinny Monthly Notices of the Royal Astronomical Society 499(3) 3706 (2020) https://doi.org/10.1093/mnras/staa3099
Observational constraints on the origin of the elements
Elemental abundances of M dwarfs based on high-resolution near-infrared spectra: Verification by binary systems
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The Gaia-ESO Survey: a new approach to chemically characterising young open clusters
The nearby magnetic cool DZ white dwarf PM J08186−3110
Adela Kawka, Stéphane Vennes, Nicole F Allard, T Leininger and F X Gadéa Monthly Notices of the Royal Astronomical Society 500(2) 2732 (2020) https://doi.org/10.1093/mnras/staa3421
The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations
Study of the departures from LTE in the unevolved stars infrared spectra
E Oliva, P Bonifacio, E Caffau, S M Andrievsky and S A Korotin Monthly Notices of the Royal Astronomical Society 496(2) 2462 (2020) https://doi.org/10.1093/mnras/staa1707
Neutral Iron Emission Lines from the Dayside of KELT-9b: The GAPS Program with HARPS-N at TNG XX
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Fast Inversion of Solar Ca ii Spectra in Non-local Thermodynamic Equilibrium
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Application of Laboratory Atomic Physics to Some Significant Stellar Chemical Composition Questions
Consistent Iron Abundances Derived from Neutral and Singly Ionized Iron Lines in Ultraviolet and Optical Spectra of Six Warm Metal-poor Stars∗
Ian U. Roederer, Christopher Sneden, James E. Lawler, Jennifer S. Sobeck, John J. Cowan and Ann Merchant Boesgaard The Astrophysical Journal 860(2) 125 (2018) https://doi.org/10.3847/1538-4357/aac6df
NLTE Line Formation for Mg i and Mg ii in the Atmospheres of B–A–F–G–K Stars
An LTE effective temperature scale for red supergiants in the Magellanic clouds
H M Tabernero, R Dorda, I Negueruela and C González-Fernández Monthly Notices of the Royal Astronomical Society 476(3) 3106 (2018) https://doi.org/10.1093/mnras/sty399
The benchmark halo giant HD 122563: CNO abundances revisited with three-dimensional hydrodynamic model stellar atmospheres
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Chemical characterization of the inner Galactic bulge:North–South symmetry
G Nandakumar, N Ryde, M Schultheis, et al. Monthly Notices of the Royal Astronomical Society 478(4) 4374 (2018) https://doi.org/10.1093/mnras/sty1255
Abundances in the Local Region. III. Southern F, G, and K Dwarfs
Berkeley 51, a young open cluster with four yellow supergiants
I Negueruela, M Monguió, A Marco, et al. Monthly Notices of the Royal Astronomical Society 477(3) 2976 (2018) https://doi.org/10.1093/mnras/sty718
Atmospheric stellar parameters for large surveys using FASMA, a new spectral synthesis package
M. Tsantaki, D. T. Andreasen, G. D. C. Teixeira, et al. Monthly Notices of the Royal Astronomical Society 473(4) 5066 (2018) https://doi.org/10.1093/mnras/stx2564
Calculation of molecular line intensity in stellar atmospheres
Fe i Oscillator Strengths for Transitions from High-lying Odd-parity Levels
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Non-local Thermodynamic Equilibrium Stellar Spectroscopy with 1D and
Models. I. Methods and Application to Magnesium Abundances in Standard Stars
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