Boris S. Kalita
A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST
Kalita, Boris S.; Yu, Si-Yue; Silverman, John D.; Daddi, Emanuele; Ho, Luis C.; Faisst, Andreas L.; Dessauges-Zavadsky, Miroslava; Puglisi, Annagrazia; Birrer, Simon; Kashino, Daichi; Ding, Xuheng; Kartaltepe, Jeyhan S.; Liu, Zhaoxuan; Kakkad, Darshan; Valentino, Francesco; Ilbert, Olivier; Magdis, Georgios; Long, Arianna S.; Jin, Shuowen; Koekemoer, Anton M.; Massey, Richard
Authors
Si-Yue Yu
John D. Silverman
Emanuele Daddi
Luis C. Ho
Andreas L. Faisst
Miroslava Dessauges-Zavadsky
Dr Annagrazia Puglisi annagrazia.puglisi@durham.ac.uk
Academic Visitor
Simon Birrer
Daichi Kashino
Xuheng Ding
Jeyhan S. Kartaltepe
Zhaoxuan Liu
Darshan Kakkad
Francesco Valentino
Olivier Ilbert
Georgios Magdis
Arianna S. Long
Shuowen Jin
Anton M. Koekemoer
Professor Richard Massey r.j.massey@durham.ac.uk
Professor
Abstract
Recent JWST observations have revealed the prevalence of spiral structures at z > 1. Unlike in the local Universe, the origin and the consequence of spirals at this epoch remain unexplored. We use public JWST/NIRCam data from the COSMOS-Web survey to map spiral structures in eight massive (>1010.5 M⊙) star-forming galaxies at zspec ∼ 1.5. We present a method for systematically quantifying spiral arms at z > 1, enabling direct measurements of flux distributions. Using rest-frame near-IR images, we construct morphological models accurately tracing spiral arms. We detect offsets (∼0.2–0.8 kpc) between the rest-frame optical and near-IR flux distributions across most arms. Drawing parallels to the local Universe, we conclude that these offsets reflect the presence of density waves. For 9 out of 18 arms, the offsets indicate spiral shocks triggered by density waves. In all, 5 arms have offsets in the opposite direction and are likely associated with tidal interactions. For the remaining cases with no detected offsets, we suggest that stochastic “clumpy” star formation is the primary driver of their formation. In conclusion, we find a multifaceted nature of spiral arms at z > 1, similar to that in the local Universe.
Citation
Kalita, B. S., Yu, S.-Y., Silverman, J. D., Daddi, E., Ho, L. C., Faisst, A. L., Dessauges-Zavadsky, M., Puglisi, A., Birrer, S., Kashino, D., Ding, X., Kartaltepe, J. S., Liu, Z., Kakkad, D., Valentino, F., Ilbert, O., Magdis, G., Long, A. S., Jin, S., Koekemoer, A. M., & Massey, R. (2025). A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST. Astrophysical Journal Letters, 979(2), Article L44. https://doi.org/10.3847/2041-8213/ada958
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 2, 2025 |
Online Publication Date | Jan 29, 2025 |
Publication Date | Feb 1, 2025 |
Deposit Date | Feb 14, 2025 |
Publicly Available Date | Feb 14, 2025 |
Journal | The Astrophysical Journal Letters |
Print ISSN | 2041-8205 |
Electronic ISSN | 2041-8213 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 979 |
Issue | 2 |
Article Number | L44 |
DOI | https://doi.org/10.3847/2041-8213/ada958 |
Keywords | Spiral galaxies, Galaxy evolution |
Public URL | https://durham-repository.worktribe.com/output/3364110 |
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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
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