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Ionized-gas Metallicity of the Strong [O iii]λ5007 Emission-line Compact Galaxies in the LAMOST Survey
Siqi 思琦 Liu 刘, A-Li 阿理 Luo 罗, Wei 伟 Zhang 张, Xiao 啸 Kong 孔, Yan-Xia 彦霞 Zhang 张, Shi-Yin 世银 Shen 沈 and Yong-Heng 永恒 Zhao 赵 The Astrophysical Journal Supplement Series 267(1) 16 (2023) https://doi.org/10.3847/1538-4365/acd69c
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Measuring chemical abundances in AGN from infrared nebular lines: HII-CHI-MISTRY-IR for AGN
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Nitrogen evolution in the halo, thick disc, thin disc, and bulge of the Galaxy
Metal-poor Stars Observed with the Automated Planet Finder Telescope. I. Discovery of Five Carbon-enhanced Metal-poor Stars from LAMOST
Mohammad K. Mardini, Haining Li, Vinicius M. Placco, Sofya Alexeeva, Daniela Carollo, Ali Taani, Iminhaji Ablimit, Liang Wang and Gang Zhao The Astrophysical Journal 875(2) 89 (2019) https://doi.org/10.3847/1538-4357/ab0fa2
Evolution of N/O ratios in galaxies from cosmological hydrodynamical simulations
Elisabeth Vangioni, Irina Dvorkin, Keith A Olive, et al. Monthly Notices of the Royal Astronomical Society 477(1) 56 (2018) https://doi.org/10.1093/mnras/sty559
Extragalactic archaeology with the C, N, and O chemical abundances
Nitrogen and oxygen abundances in the Local Universe
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RADIAL TRENDS IN IMF-SENSITIVE ABSORPTION FEATURES IN TWO EARLY-TYPE GALAXIES: EVIDENCE FOR ABUNDANCE-DRIVEN GRADIENTS
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Modeling the chemical evolution of the Galaxy halo
Stellar mass loss, rotation and the chemical enrichment of early-type galaxies
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CONSTRAINING THE STAR FORMATION HISTORIES OF GAMMA-RAY BURST HOST GALAXIES FROM THEIR OBSERVED ABUNDANCE PATTERNS
Francesco Calura, Miroslava Dessauges-Zavadski, Jason X. Prochaska and Francesca Matteucci The Astrophysical Journal 693(2) 1236 (2009) https://doi.org/10.1088/0004-637X/693/2/1236
Nucleosynthesis from massive stars 50 years after B2FH
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Georges Meynet, Cristina Chiappini, Cyril Georgy, et al. Proceedings of the International Astronomical Union 4(S254) 325 (2008) https://doi.org/10.1017/S1743921308027774
A new imprint of fast rotators: low
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Population Synthesis in the Blue. IV. Accurate Model Predictions for Lick Indices and
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Formation and evolution of the Galactic bulge: constraints from stellar abundances
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