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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

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Authors

Boris S. Kalita

Si-Yue Yu

John D. Silverman

Emanuele Daddi

Luis C. Ho

Andreas L. Faisst

Miroslava Dessauges-Zavadsky

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



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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