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Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si − III. Grids of isochrones for −2.5 ≤ [Fe/H] ≤ −0.5 and helium abundances Y = 0.25 and 0.29 at each metallicity
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Staring at the Shadows of Archaic Galaxies: Damped Lyα and Metal Absorbers Toward a Young z ∼ 6 Weak-line Quasar
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When did the initial mass function become bottom-heavy?
The COS Absorption Survey of Baryon Harbors: unveiling the physical conditions of circumgalactic gas through multiphase Bayesian ionization modelling
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The Cosmic Ultraviolet Baryon Survey (CUBS) – III. Physical properties and elemental abundances of Lyman-limit systems at z < 1
Fakhri S Zahedy, Hsiao-Wen Chen, Thomas M Cooper, et al. Monthly Notices of the Royal Astronomical Society 506(1) 877 (2021) https://doi.org/10.1093/mnras/stab1661
The CARMENES search for exoplanets around M dwarfs
Models of metal-poor stars with different initial abundances of C, N, O, Mg, and Si – I. Bolometric corrections derived from new MARCS synthetic spectra and their implications for observed colour–magnitude diagrams
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The Chemical Evolution of Carbon, Nitrogen, and Oxygen in Metal-poor Dwarf Galaxies
Danielle A. Berg, Dawn K. Erb, Richard B. C. Henry, Evan D. Skillman and Kristen B. W. McQuinn The Astrophysical Journal 874(1) 93 (2019) https://doi.org/10.3847/1538-4357/ab020a
The Most Metal-poor Stars. V. The CEMP-no Stars in 3D and Non-LTE
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Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. III. M55 and NGC 6362
Friedrich-Karl Thielemann, Roland Diehl, Alexander Heger, Raphael Hirschi and Matthias Liebendörfer Astrophysics and Space Science Library, Astrophysics with Radioactive Isotopes 453 173 (2018) https://doi.org/10.1007/978-3-319-91929-4_4
Carbon Abundances in Starburst Galaxies of the Local Universe
María A. Peña-Guerrero, Claus Leitherer, Selma de Mink, Aida Wofford and Lisa Kewley The Astrophysical Journal 847(2) 107 (2017) https://doi.org/10.3847/1538-4357/aa88bf
Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937
CARBON AND OXYGEN ABUNDANCES IN LOW METALLICITY DWARF GALAXIES
Danielle A. Berg, Evan D. Skillman, Richard B. C. Henry, Dawn K. Erb and Leticia Carigi The Astrophysical Journal 827(2) 126 (2016) https://doi.org/10.3847/0004-637X/827/2/126
Chemical abundances in high-redshift galaxies: a powerful new emission line diagnostic
The Galactic chemical evolution of oxygen inferred from 3D non-LTE spectral-line-formation calculations
A. M. Amarsi, M. Asplund, R. Collet and J. Leenaarts Monthly Notices of the Royal Astronomical Society: Letters 454(1) L11 (2015) https://doi.org/10.1093/mnrasl/slv122
COLOR–MAGNITUDE DIAGRAM CONSTRAINTS ON THE METALLICITIES, AGES, AND STAR FORMATION HISTORY OF THE STELLAR POPULATIONS IN THE CARINA DWARF SPHEROIDAL GALAXY
Reionisation and High-Redshift Galaxies: The View from Quasar Absorption Lines
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Australia 32 (2015) https://doi.org/10.1017/pasa.2015.45
Ultraviolet emission lines in young low-mass galaxies at z ≃ 2: physical properties and implications for studies at z > 7
Daniel P. Stark, Johan Richard, Brian Siana, et al. Monthly Notices of the Royal Astronomical Society 445(3) 3200 (2014) https://doi.org/10.1093/mnras/stu1618
THEs-PROCESS ENRICHMENT OF THE GLOBULAR CLUSTERS M4 AND M22
Molecular hydrogen from z = 0.0963 DLA towards the QSO J1619+3342★
R. Srianand, H. Rahmani, S. Muzahid and V. Mohan Monthly Notices of the Royal Astronomical Society 443(4) 3318 (2014) https://doi.org/10.1093/mnras/stu1405
The chemical composition of a regular halo globular cluster: NGC 5897
Carbon and oxygen abundances from recombination lines in low-metallicity star-forming galaxies. Implications for chemical evolution★
C. Esteban, J. García-Rojas, L. Carigi, et al. Monthly Notices of the Royal Astronomical Society 443(1) 624 (2014) https://doi.org/10.1093/mnras/stu1177
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COSMOLOGICAL SIMULATIONS OF INTERGALACTIC MEDIUM EVOLUTION. I. TEST OF THE SUBGRID CHEMICAL ENRICHMENT MODEL
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The First Stars: clues from quasar absorption systems
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[O/Fe] ESTIMATES FOR CARBON-ENHANCED METAL-POOR STARS FROM NEAR-INFRARED SPECTROSCOPY
F.-K. Thielemann, R. Hirschi, M. Liebendörfer and R. Diehl Lecture Notes in Physics, Astronomy with Radioactivities 812 153 (2011) https://doi.org/10.1007/978-3-642-12698-7_4
The most metal-poor damped Lyα systems: insights into chemical evolution in the very metal-poor regime★
Ryan Cooke, Max Pettini, Charles C. Steidel, Gwen C. Rudie and Poul E. Nissen Monthly Notices of the Royal Astronomical Society 417(2) 1534 (2011) https://doi.org/10.1111/j.1365-2966.2011.19365.x
An absolutely calibratedTeffscale from the infrared flux method