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Chemical Abundances and Galaxy Evolution [PDF]
, 1984 The chemical abundance characteristics of two comparatively structurally simple classes of galaxies, the ellipticals and irregulars, are briefly reviewed. Neither of these types of galaxies have properties which are fully consistent with the quantitative predictions of basic chemical evolution models. Possible sources for discrepancies are discussed in
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Chemical Abundances in Old Populations
1992Preliminary single-burst population synthesis models are presented for weak and strong spectral features as a function of metallicity for old populations. Models agree with published globular cluster observations as well as theoretical calibrations. For small ellipticals, the galaxies and model predictions agree well in all indices.
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The chemical abundances of the Ap star HD94660
AIP Conference Proceedings, 2014In this work I present the determination of chemical abundances of the Ap star HD94660, a possible rapid oscillating star. As all the magnetic chemically peculiar objects, it presents CNO underabundance and overabundance of iron peak elements of ∼100 times and of rare earths up to 4 dex with respect to the Sun.
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Direct observation of chemical short-range order in a medium-entropy alloy
Nature, 2021Lingling Zhou, Qiqi Xue, Fuping Yuan
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Chemical Bonding in Chalcogenides: The Concept of Multicenter Hyperbonding
Advanced Materials, 2020Stephen R Elliott
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Chemical Bonding and Bonding Models of Main-Group Compounds
Chemical Reviews, 2019Gernot Frenking +2 more
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