Changbom Park
Formation and Morphology of the First Galaxies in the Cosmic Morning
Park, Changbom; Lee, Jaehyun; Kim, Juhan; Jeong, Donghui; Pichon, Christophe; Gibson, Brad K.; Snaith, Owain N.; Shin, Jihye; Kim, Yonghwi; Dubois, Yohan; Few, C. Gareth
Authors
Jaehyun Lee
Juhan Kim
Donghui Jeong
Christophe Pichon
Brad K. Gibson
Owain N. Snaith
Jihye Shin
Yonghwi Kim
Yohan Dubois
Dr Gareth Few G.Few@hull.ac.uk
Lecturer
Abstract
We investigate the formation and morphological evolution of the first galaxies in the cosmic morning (10 ≳ z ≳ 4) using the Horizon Run 5 (HR5) simulation. For galaxies above the stellar mass M ⋆ , min = 2 × 10 9 M ⊙ , we classify them into disk, spheroid, and irregular types according to their asymmetry and stellar-mass morphology. We find that about two-thirds of the galaxies have a Sérsic index <1.5, reflecting the dominance of disk-type morphology in the cosmic morning. The rest are evenly distributed as incidental and transient irregulars or spheroids. These fractions are roughly independent of redshift and stellar mass up to ∼1010 M ⊙. Almost all the first galaxies with M ⋆ > M ⋆ , min at z > 4 form at initial peaks of the matter-density field. Large-scale structures in the universe emerge and grow like cosmic rhizomes as the underlying matter-density fluctuations grow and form associations of galaxies in rare overdense regions and the realm of the galactic world is stretched into relatively lower-density regions along evolving filaments. The cosmic web of galaxies forms at lower redshifts when most rhizomes globally percolate. The primordial angular momentum produced by the induced tidal torques on protogalactic regions is correlated with the internal kinematics of galaxies and tightly aligned with the angular momentum of the total galaxy mass. The large-scale tidal field imprinted in the initial conditions seems responsible for the dominance of disk morphology and for the tendency of galaxies to reacquire a disk postdistortion.
Citation
Park, C., Lee, J., Kim, J., Jeong, D., Pichon, C., Gibson, B. K., …Few, C. G. (2022). Formation and Morphology of the First Galaxies in the Cosmic Morning. The Astrophysical journal, 937(1), https://doi.org/10.3847/1538-4357/ac85b5
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 27, 2022 |
Online Publication Date | Sep 16, 2022 |
Publication Date | Sep 20, 2022 |
Deposit Date | Dec 10, 2022 |
Publicly Available Date | Dec 15, 2022 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Electronic ISSN | 1538-4357 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 937 |
Issue | 1 |
DOI | https://doi.org/10.3847/1538-4357/ac85b5 |
Public URL | https://hull-repository.worktribe.com/output/4095017 |
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Copyright Statement
© 2022. The Author(s). Published by the American Astronomical Society.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
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