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Spatially Resolved UV Nebular Diagnostics in Star-Forming Galaxies

Published onMay 31, 2019
Spatially Resolved UV Nebular Diagnostics in Star-Forming Galaxies
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Abstract

This paper describes the need for spatially resolved rest-frame UV spectroscopy across nearby SFGs via a space-based UV-IFU. Such observations will robustly constrain the diagnostic tools critical to understanding fundamental questions concerning the evolution, physical conditions, and ionization structure of SFGs across cosmic time.

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