http://arxiv.org/abs/2005.06054
Diffuse ionized gas (DIG) in galaxies can be found in early-type galaxies, in bulges of late-type galaxies, in the interarm regions of galaxy disks, and outside the plane of such disks. The emission-line spectrum of the DIG can be confused with that of a weakly active galactic nucleus. It can also bias the inference of chemical abundances and star formation rates in star forming galaxies. We discuss how one can detect and feasibly correct for the DIG contribution in galaxy spectra.
N. Asari and G. Stasińska
Thu, 14 May 20
35/56
Comments: 8 pages, 6 figures, Invited review, Proceedings of IAUS 359, Storchi-Bergmann et al. eds
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