Aristeidis Amvrosiadis aristeidis.amvrosiadis@durham.ac.uk
Post Doctoral Research Associate
Aristeidis Amvrosiadis aristeidis.amvrosiadis@durham.ac.uk
Post Doctoral Research Associate
Sam Lange samuel.c.lange@durham.ac.uk
PGR Student Doctor of Philosophy
James Nightingale james.w.nightingale@durham.ac.uk
Academic Visitor
Dr Qiuhan He qiuhan.he@durham.ac.uk
Post Doctoral Research Associate
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Dr Kyle Oman kyle.a.oman@durham.ac.uk
Associate Professor - Royal Society Dorothy Hodgkin Fellow
Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
Professor Mark Swinbank a.m.swinbank@durham.ac.uk
Professor
Dr Francesca Fragkoudi francesca.fragkoudi@durham.ac.uk
Associate Professor
Dr Dimitri Gadotti dimitri.a.gadotti@durham.ac.uk
Associate Professor
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
E. Borsato
A. Robertson
Professor Richard Massey r.j.massey@durham.ac.uk
Professor
X. Cao
R. Li
We examine the morphological and kinematical properties of SPT-2147, a strongly lensed, massive, dusty, star-forming galaxy at z = 3.762. Combining data from JWST, Hubble Space Telescope, and ALMA, we study the galaxy’s stellar emission, dust continuum, and gas properties. The imaging reveals a central bar structure in the stars and gas embedded within an extended disc with a spiral arm-like feature. The kinematics confirm the presence of the bar and of the regularly rotating disc. Dynamical modelling yields a dynamical mass, Mdyn = (9.7 ± 2.0) × 1010M☉, and a maximum rotational velocity to velocity dispersion ratio, V / σ = 9.8 ± 1.2. From multiband imaging we infer, via spectral energy distribution fitting, a stellar mass, M⋆ = (6.3 ± 0.9) × 1010M☉, and a star formation rate, SFR = 781 ± 99M☉ yr-1, after correcting for magnification. Combining these measurements with the molecular gas mass, we derive a baryonic-to-total mass ratio of Mbar / Mdyn = 1.1 ± 0.3 within 4.0 kpc. This finding suggests that the formation of bars in galaxies begins earlier in the history of the Universe than previously thought and can also occur in galaxies with elevated gas fractions.
Amvrosiadis, A., Lange, S., Nightingale, J. W., He, Q., Frenk, C. S., Oman, K. A., Smail, I., Swinbank, A. M., Fragkoudi, F., Gadotti, D. A., Cole, S., Borsato, E., Robertson, A., Massey, R., Cao, X., & Li, R. (2025). The onset of bar formation in a massive galaxy at z ∼ 3.8. Monthly Notices of the Royal Astronomical Society, 537(2), 1163-1181. https://doi.org/10.1093/mnras/staf048
Journal Article Type | Article |
---|---|
Acceptance Date | Dec 16, 2024 |
Online Publication Date | Jan 11, 2025 |
Publication Date | Feb 1, 2025 |
Deposit Date | Apr 7, 2025 |
Publicly Available Date | Apr 7, 2025 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 537 |
Issue | 2 |
Pages | 1163-1181 |
DOI | https://doi.org/10.1093/mnras/staf048 |
Public URL | https://durham-repository.worktribe.com/output/3781911 |
Published Journal Article
(3.2 Mb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
FLASH: Faint Lenses from Associated Selection with Herschel
(2023)
Journal Article
Abell 1201: detection of an ultramassive black hole in a strong gravitational lens
(2023)
Journal Article
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
Apache License Version 2.0 (http://www.apache.org/licenses/)
Apache License Version 2.0 (http://www.apache.org/licenses/)
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search