The reports of thick discs' deaths are greatly exaggerated: thick discs are NOT artefacts caused by diffuse scattered light
S\'ebastien Comer\'on, Heikki Salo, Johan H. Knapen

TL;DR
This study re-evaluates the nature of thick discs in galaxies, demonstrating they are not artifacts of scattered light but are indeed common features with significant mass, challenging previous assumptions.
Contribution
The paper introduces an improved point spread function model that confirms the ubiquity of thick discs and clarifies their properties, countering earlier claims of their being artifacts.
Findings
Thick discs are nearly ubiquitous in edge-on galaxies.
Scattered light from thin discs dominates surface brightness below 26 mag/arcsec^2.
Thick discs have comparable masses to thin discs in low-mass galaxies.
Abstract
Recent studies have made the community aware of scattered light when examining low-surface-brightness galaxy features such as thick discs. In our past studies of the thick discs of edge-on galaxies in the Spitzer Survey of Stellar Structure in Galaxies (SG) we modelled the point spread function as a Gaussian. We re-examine our results using a revised point spread function model that accounts for extended wings out to more than 2.5arcmin. We study the images of 141 edge-on galaxies from the SG. We decompose the surface brightness profiles of the galaxies perpendicular to their mid-planes assuming that discs are made of two stellar discs in hydrostatic equilibrium. We decompose the axial surface brightness profiles of galaxies to model the central mass concentration - described by a S\'ersic function - and the disc - described by a broken exponential disc. Our…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
