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Metal Abundances and Depletions in the Neutral Interstellar Medium of Galaxies: the Local Volume as a Laboratory

Published onMay 31, 2019
Metal Abundances and Depletions in the Neutral Interstellar Medium of Galaxies: the Local Volume as a Laboratory
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Abstract

Multi-object UV-optical spectroscopy toward massive stars within 15 Mpc covering a wide range of metallicities and morphological types will provide the abundance measurements needed to characterize the lifecycle of metals in neutral gas and dust in galaxies, thereby addressing important questions about chemical enrichment.

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