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Investigating the Origin of Observed Central Dips in Radial Metallicity Profiles
[article]
2022
arXiv
pre-print
Radial metallicity trends provide a key indicator of physical processes such as star formation and radial gas migration within a galaxy. Large IFU surveys allow for detailed studies of these radial variations, with recent observations detecting central dips in the metallicity, which may trace the impact of various evolutionary processes. However, the origin of these dips has not been conclusively determined, with suggestions that they may be diagnostic dependent. In this paper, we use the
arXiv:2201.03296v1
fatcat:7rlt2pd6bbacpl53hwkkaqasdm