Chemodynamical Model of the Galaxy: Abundance Gradients Predicted for H
Christine Allen+2 more
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Abundances of Red Giants in the Andromeda II Dwarf Spheroidal Galaxy [PDF]
Patrick Côté+2 more
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Gas-phase metallicity gradients are a crucial element in understanding the chemical evolution of galaxies. We use the FOGGIE simulations to study the metallicity gradients (∇ Z ) of six Milky Way–like galaxies throughout their evolution.
Ayan Acharyya+9 more
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Chemical Abundances of Planetary Nebulae in the Sagittarius Dwarf Elliptical Galaxy [PDF]
J. R. Walsh+3 more
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Two-process Model and Residual Abundance Analysis of the Milky Way Massive Satellites
The “two-process model” is a promising technique for interpreting stellar chemical abundance data from large-scale surveys (e.g., the Sloan Digital Sky Survey IV/V and the Galactic Archeology with HERMES survey), enabling more quantitative empirical ...
Sten Hasselquist+6 more
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Theoretical models of the planetary nebula populations in galaxies: The ISM oxygen abundance when star formation stops [PDF]
M. G. Richer, M. L. McCall, N. Arimoto
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Oxygen Abundances in Diffuse Ellipticals and the Metallicity-Luminosity Relation for Dwarf Galaxies [PDF]
M. G. Richer, M. L. McCall, N. Arimoto
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On the Evolutionary History of a Simulated Disk Galaxy as Seen by Phylogenetic Trees
Phylogenetic methods have long been used in biology and more recently have been extended to other fields—for example, linguistics and technology—to study evolutionary histories.
Danielle de Brito Silva+14 more
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Lack of Evolution in the Iron Abundance in Clusters of Galaxies and Implications for the Global Star Formation Rate at High Redshift [PDF]
R. F. Mushotzky, M. Loewenstein
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Abundance gradients in the Galaxy derived from H II regions
M. Peimbert+2 more
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