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Accurate abundance analysis of late-type stars: advances in atomic physics

The Astronomy and Astrophysics Review, 2016-12, Vol.24 (1), p.1-54, Article 9

Barklem, Paul S.

2016

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A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu ii and Zn ii Lines

The Astrophysical journal, 2018-04, Vol.857 (1), p.2

2018

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Correspondence between the surface integral and linear combination of atomic orbitals methods for ionic-covalent interactions in mutual neutralization processes involving H − / D

Physical review. A, 2021-12, Vol.104 (6), Article 062806

Barklem, Paul S.

2021

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State-Resolved Mutual Neutralization of Mg^{+} and D^{-}

Physical review letters, 2022-01, Vol.128 (3), p.033401-033401, Article 033401

2022

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Inelastic silicon-hydrogen collision data for non-LTE applications in stellar atmospheres

Astronomy and astrophysics (Berlin), 2014-12, Vol.572, p.1-7

2014

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The Frequency of Carbon-enhanced Metal-poor Stars in the Galaxy from the HERES Sample

The Astrophysical journal, 2006-11, Vol.652 (1), p.L37-L40

2006

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Mutual neutralisation of O with O: investigation of the role of metastable ions in a combined experimental and theoretical study

Physical chemistry chemical physics : PCCP, 2021-11, Vol.23 (43), p.2467-24616

2021

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Erratum: State-Resolved Mutual Neutralization of Mg^{+} and D^{-} [Phys. Rev. Lett. 128, 033401 (2022)]

Physical review letters, 2023-01, Vol.130 (2), p.029901-029901, Article 029901

2023

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Nucleosynthetic signatures of the first stars

Nature, 2005-04, Vol.434 (7035), p.871-873

2005

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Lithium Abundances of Extremely Metal-Poor Turnoff Stars

The Astrophysical journal, 2009-06, Vol.698 (2), p.1803-1812

2009

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Partition functions and equilibrium constants for diatomic molecules and atoms of astrophysical interest

Astronomy and astrophysics (Berlin), 2016-04, Vol.588, p.A96

2016

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Final-state-resolved mutual neutralization of Na + and D

Physical review. A, 2021-03, Vol.103 (3), Article 032814

2021

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Excitation and charge transfer in low-energy hydrogen atom collisions with neutral iron

Astronomy and astrophysics (Berlin), 2018-04, Vol.612, p.A90

Barklem, P. S.

2018

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Observation of an isotope effect in state-selective mutual neutralization of lithium with hydrogen

Physical review. A, 2023-10, Vol.108 (4), Article 042810

2023

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Hydrogen Atom Collision Processes in Cool Stellar Atmospheres: Effects on Spectral Line Strengths and Measured Chemical Abundances in Old Stars

Journal of physics. Conference series, 2012-01, Vol.397 (1), p.1-7

Barklem, Paul S

2012

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Non-LTE line formation of Fe in late-type stars – III. 3D non-LTE analysis of metal-poor stars

Monthly notices of the Royal Astronomical Society, 2016-12, Vol.463 (2), p.1518-1518

2016

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Excitation and charge transfer in low-energy hydrogen atom collisions with neutral oxygen

Astronomy and astrophysics (Berlin), 2018-02, Vol.610, p.A57

Barklem, P. S.

2018

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Revisiting the statistical equilibrium of H- in stellar atmospheres

Astronomy and astrophysics (Berlin), 2024-08

2024

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3D non-LTE line formation of neutral carbon in the Sun

Astronomy and astrophysics (Berlin), 2019-04, Vol.624, p.A111

2019

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Excitation and charge transfer in low-energy hydrogen-atom collisions with neutral atoms: Theory, comparisons, and application to Ca

Physical review. A, 2016-04, Vol.93 (4), Article 042705

Barklem, Paul S.

2016

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Non-LTE calculations for neutral Na in late-type stars using improved atomic data

Astronomy and astrophysics (Berlin), 2011-04, Vol.528, p.A103

2011

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A collection of model stellar spectra for spectral types B to early-M

Astronomy and astrophysics (Berlin), 2018-10, Vol.618, p.A25

2018

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Inelastic O plus H collisions and the O I 777 nm solar centre-to-limb variation

Astronomy and astrophysics (Berlin), 2018-08, Vol.616

2018

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3D NLTE analysis of the most iron-deficient star, SMSS0313-6708

Astronomy and astrophysics (Berlin), 2017-01, Vol.597, p.A6

2017

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Mg line formation in late-type stellar atmospheres: II. Calculations in a grid of 1D models

Astronomy and astrophysics (Berlin), 2016-02, Vol.586, p.A120

2016

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Accurate abundance analysis of late-type stars: advances in atomic physics

A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu ii and Zn ii Lines

Correspondence between the surface integral and linear combination of atomic orbitals methods for ionic-covalent interactions in mutual neutralization processes involving H − / D

State-Resolved Mutual Neutralization of Mg^{+} and D^{-}

Inelastic silicon-hydrogen collision data for non-LTE applications in stellar atmospheres

The Frequency of Carbon-enhanced Metal-poor Stars in the Galaxy from the HERES Sample

Mutual neutralisation of O with O: investigation of the role of metastable ions in a combined experimental and theoretical study

Erratum: State-Resolved Mutual Neutralization of Mg^{+} and D^{-} [Phys. Rev. Lett. 128, 033401 (2022)]

Nucleosynthetic signatures of the first stars

Lithium Abundances of Extremely Metal-Poor Turnoff Stars

Partition functions and equilibrium constants for diatomic molecules and atoms of astrophysical interest

Final-state-resolved mutual neutralization of Na + and D

Excitation and charge transfer in low-energy hydrogen atom collisions with neutral iron

Observation of an isotope effect in state-selective mutual neutralization of lithium with hydrogen

Hydrogen Atom Collision Processes in Cool Stellar Atmospheres: Effects on Spectral Line Strengths and Measured Chemical Abundances in Old Stars

Non-LTE line formation of Fe in late-type stars – III. 3D non-LTE analysis of metal-poor stars

Excitation and charge transfer in low-energy hydrogen atom collisions with neutral oxygen

Revisiting the statistical equilibrium of H- in stellar atmospheres

3D non-LTE line formation of neutral carbon in the Sun

Excitation and charge transfer in low-energy hydrogen-atom collisions with neutral atoms: Theory, comparisons, and application to Ca

Non-LTE calculations for neutral Na in late-type stars using improved atomic data

A collection of model stellar spectra for spectral types B to early-M

Inelastic O plus H collisions and the O I 777 nm solar centre-to-limb variation

3D NLTE analysis of the most iron-deficient star, SMSS0313-6708

Mg line formation in late-type stellar atmospheres: II. Calculations in a grid of 1D models

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