Diverse structural evolution at z > 1 in cosmologically simulated galaxies

Gregory F. Snyder*, Jennifer Lotz, Christopher Moody, Michael Peth, Peter Freeman, Daniel Ceverino, Joel Primack, Avishai Dekel

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

61 Scopus citations

Abstract

From mock Hubble Space Telescope images, we quantify non-parametric statistics of galaxy morphology, thereby predicting the emergence of relationships among stellar mass, star formation, and observed rest-frame optical structure at 1<z<3.We measure automated diagnostics of galaxy morphology in cosmological simulations of the formation of 22 central galaxies with 9.3 < log10M*/M < 10.7. These high-spatial-resolution zoom-in calculations enable accurate modelling of the rest-frame UV and optical morphology. Even with small numbers of galaxies, we find that structural evolution is neither universal nor monotonic: galaxy interactions can trigger either bulge or disc formation, and optically bulge-dominated galaxies at this mass may not remain so forever. Simulated galaxies with M* > 1010M contain relatively more disc-dominated light profiles than those with lower mass, reflecting significant disc brightening in some haloes at 1 < z < 2. By this epoch, simulated galaxies with specific star formation rates below 10-9.7 yr-1 are more likely than normal star-formers to have a broader mix of structural types, especially atM* > 1010M. We analyse a cosmological major merger at z ~ 1.5 and find that the newly proposed Multimode-Intensity-Deviation (MID) morphology diagnostics trace later merger stages while Gini-M20 trace earlier ones. MID is sensitive also to clumpy star-forming discs. The observability time of typical MID-enhanced events in our simulation sample is <100 Myr. A larger sample of cosmological assembly histories may be required to calibrate such diagnostics in the face of their sensitivity to viewing angle, segmentation algorithm, and various phenomena such as clumpy star formation and minor mergers.

Original languageEnglish
Pages (from-to)4290-4310
Number of pages21
JournalMonthly Notices of the Royal Astronomical Society
Volume451
Issue number4
DOIs
StatePublished - 24 Apr 2015

Bibliographical note

Publisher Copyright:
© 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.

Keywords

  • Galaxies: formation
  • Galaxies: structure
  • Methods: numerical

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