Simulating galaxies in the reionization era with FIRE-2: Morphologies and sizes

Xiangcheng Ma, Philip F. Hopkins, Michael Boylan-Kolchin, Claude André Faucher-Giguère, Eliot Quataert, Robert Feldmann, Shea Garrison-Kimmel, Christopher C. Hayward, Dušan Kereš, Andrew Wetzel

Research output: Contribution to journalArticle

15 Scopus citations

Abstract

We study the morphologies and sizes of galaxies at z ≥ 5 using high-resolution cosmological zoom-in simulations from the Feedback In Realistic Environments project. The galaxies show a variety of morphologies, from compact to clumpy to irregular. The simulated galaxies have more extended morphologies and larger sizes when measured using rest-frame optical B-band light than rest-frameUVlight; sizes measured from stellarmass surface density are even larger. The UV morphologies are usually dominated by several small, bright young stellar clumps that are not always associated with significant stellarmass. The B-band light traces stellarmass better than the UV, but it can also be biased by the bright clumps. At all redshifts, galaxy size correlates with stellar mass/luminosity with large scatter. The half-light radii range from 0.01 to 0.2 arcsec (0.05-1 kpc physical) at fixed magnitude. At z ≥ 5, the size of galaxies at fixed stellar mass/luminosity evolves as (1 + z)-m, with m ~ 1-2. For galaxies less massive than M* ~ 108M, the ratio of the half-mass radius to the halo virial radius is ~10 per cent and does not evolve significantly at z = 5-10; this ratio is typically 1-5 per cent for more massive galaxies. A galaxy's 'observed' size decreases dramatically at shallower surface brightness limits. This effect may account for the extremely small sizes of z ≥ 5 galaxies measured in the Hubble Frontier Fields. We provide predictions for the cumulative light distribution as a function of surface brightness for typical galaxies at z = 6.

Original languageEnglish (US)
Pages (from-to)219-229
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume477
Issue number1
DOIs
StatePublished - Jun 11 2018
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Cosmology: Theory
  • Galaxies: Evolution
  • Galaxies: Formation
  • Galaxies: High-redshift

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    Ma, X., Hopkins, P. F., Boylan-Kolchin, M., Faucher-Giguère, C. A., Quataert, E., Feldmann, R., Garrison-Kimmel, S., Hayward, C. C., Kereš, D., & Wetzel, A. (2018). Simulating galaxies in the reionization era with FIRE-2: Morphologies and sizes. Monthly Notices of the Royal Astronomical Society, 477(1), 219-229. https://doi.org/10.1093/mnras/sty684