Chemical Evolution of Galaxies: Abundance Trends and Implications [PDF]
James W. Truran
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Determining Stellar Elemental Abundances from DESI Spectra with the Data-driven Payne
Stellar abundances for a large number of stars provide key information for the study of Galactic formation history. Large spectroscopic surveys such as the Dark Energy Spectroscopic Instrument (DESI) and LAMOST take median-to-low-resolution ( R ≲ 5000 ...
Meng Zhang+10 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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A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii
A near-infrared spectrum of nova V1716 Scorpii (PNV J17224490-4137160), a recent bright ( ${V}_{\max }=7.3$ mag), Fermi-LAT detected γ -ray source, was modeled using the photoionization code CLOUDY.
C. E. Woodward+4 more
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CHEMTAX - a program for estimating class abundances from chemical markers:application to HPLC measurements of phytoplankton [PDF]
M.D. Mackey+3 more
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Chemical abundances and ionizing clusters of H ii regions in the LINER galaxy NGC 4258 [PDF]
Á. I. Díaz+3 more
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Metal Abundances at [FORMULA][F]z<1.5[/F][/FORMULA]: Fresh Clues to the Chemical Enrichment History of Damped [CLC]Ly[/CLC]α Systems [PDF]
Max Pettini+3 more
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Chemical Abundance Calibrations for the Narrow-Line Region of Active Galaxies [PDF]
Thaisa Storchi‐Bergmann+3 more
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Stellar Abundances at the Center of Early-type Galaxies with Fine Structure
Our understanding of early-type galaxies (ETGs) has grown in the past decade with the advance of full-spectrum fitting techniques used to infer the properties of the stellar populations that make up the galaxy.
Nicholas Barth+4 more
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On the Chemical Abundances of Multiple‐Shell Planetary Nebulae with Halos [PDF]
M. A. Guerrero, A. Manchado
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