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Element Abundances in Nearby Galaxies

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arxiv astro-ph/0211148 v1 pith:KRKTTBEG submitted 2002-11-07 astro-ph

Donald R. Garnett (Steward Observatory , University of Arizona) This is my paper · ORCID
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keywords galaxiesabundancesassociatedelementissuesnearbyabundanceastrophysical
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In these lectures I present a highly opinionated review of the observed patterns of metallicity and element abundance ratios in nearby spiral, irregular, and dwarf elliptical galaxies, with connection to a number of astrophysical issues associated with chemical evolution. I also discuss some of the observational and theoretical issues associated with measuring abundances in H II regions and gas and stellar surface densities in disk galaxies. Finally, I will outline a few open questions that deserve attention in future investigations.

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Cited by 1 Pith paper

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  1. The JWST EXCELS survey: Probing strong-line diagnostics and the chemical evolution of galaxies over cosmic time using Te-metallicities

    astro-ph.GA 2025-02 conditional novelty 6.0 of 10

    A new neon-plus-oxygen line ratio, RNe, is introduced and validated as a largely redshift-independent metallicity diagnostic for JWST/NIRSpec out to z~11.2.

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