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The onset of bar formation in a massive galaxy at z ∼ 3.8

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.

The onset of bar formation in a massive galaxy at z ∼ 3.8 Thumbnail


Authors

Profile image of Sam Lange

Sam Lange samuel.c.lange@durham.ac.uk
PGR Student Doctor of Philosophy

Profile image of Qiuhan He

Dr Qiuhan He qiuhan.he@durham.ac.uk
Post Doctoral Research Associate

Profile image of Kyle Oman

Dr Kyle Oman kyle.a.oman@durham.ac.uk
Associate Professor - Royal Society Dorothy Hodgkin Fellow

Profile image of Ian Smail

Ian Smail ian.smail@durham.ac.uk
Emeritus Professor

E. Borsato

A. Robertson

X. Cao

R. Li



Abstract

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.

Citation

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

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