The formation and evolution of low-surface-brightness galaxies. Issue 1 (23rd February 2019)

• Record Type: Journal Article
• Authors: Martin, G; Kaviraj, S; Laigle, C; Devriendt, J E G; Jackson, R A; Peirani, S; Dubois, Y; Pichon, C; Slyz, A
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 485:Issue 1(2019)
• Page Start: 796
• Page End: 818
• Publication Date: 2019-02-23
• Subjects: Galaxies: evolution -- formation -- dwarf -- structure; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz356
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Our statistical understanding of galaxy evolution is fundamentally driven by objects that lie above the surface-brightness limits of current wide-area surveys (μ ∼ 23 mag arcsec −2 ). While both theory and small, deep surveys have hinted at a rich population of low-surface-brightness galaxies (LSBGs) fainter than these limits, their formation remains poorly understood. We use Horizon-AGN, a cosmological hydrodynamical simulation to study how LSBGs, and in particular the population of ultra-diffuse galaxies (UDGs; μ > 24.5 mag arcsec −2 ), form and evolve over time. For $M_*\gt 10^{8}\, \mathrm{M}_{\odot }$, LSBGs contribute 47, 7, and 6 per cent of the local number, mass, and luminosity densities, respectively (∼85/11/10 per cent for $M_*\gt 10^{7}\, \mathrm{M}_{\odot }$ ). Today's LSBGs have similar dark-matter fractions and angular momenta to high-surface-brightness galaxies (HSBGs; μ < 23 mag arcsec −2 ), but larger effective radii (×2.5 for UDGs) and lower fractions of dense, star-forming gas (more than ×6 less in UDGs than HSBGs). LSBGs originate from the same progenitors as HSBGs at $z$ > 2. However, LSBG progenitors form stars more rapidly at early epochs. The higher resultant rate of supernova-energy injection flattens their gas-density profiles, which, in turn, creates shallower stellar profiles that are more susceptible to tidal processes. After $z$ ∼ 1, tidal perturbations broaden LSBG stellar distributions and heat their cold gas, creating the diffuse, largely gas-poor LSBGs seen today. In clusters, ram-pressure stripping provides an additional mechanism that assists in gas removal in LSBG progenitors. Our results offer insights into the formation of a galaxy population that is central to a complete understanding of galaxy evolution, and that will be a key topic of research using new and forthcoming deep-wide surveys.