A Multiwavelength Investigation of Spiral Structures in <i>z</i> &gt; 1 Galaxies with JWST

Abstract Recent JWST observations have revealed the prevalence of spiral structures at z &gt; 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 (&gt;10 10.5 M ⊙ ) star-forming galaxies at z spec ∼ 1.5. We present a method for systematically quantifying spiral arms at z &gt; 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 &gt; 1, similar to that in the local Universe.

Authors

Institutions

Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-01-29
DOI
https://doi.org/10.3847/2041-8213/ada958
Citations
2
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
2.31

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST

Simon Birrer, Si-Yue Yu, Zhaoxuan Liu, Francesco Valentino et al.
2 citations
The Astrophysical Journal Letters
Galaxies: Formation, Evolution, Phenomena
2.31
article

A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST

Simon Birrer, Si-Yue Yu, Zhaoxuan Liu, Francesco Valentino, Darshan Kakkad, Annagrazia Puglisi, Shuowen Jin, J. D. Silverman, R. Massey, Boris S. Kalita, Anton M. Koekemoer, M. Dessauges‐Zavadsky, O. Ilbert, Luis C. Ho, G. Magdis, Emanuele Daddi, Daichi Kashino, Arianna S. Long, Jeyhan S. Kartaltepe, Andreas L. Faisst, Xuheng Ding
article en
2 citations

Abstract

Abstract Recent JWST observations have revealed the prevalence of spiral structures at z &gt; 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 (&gt;10 10.5 M ⊙ ) star-forming galaxies at z spec ∼ 1.5. We present a method for systematically quantifying spiral arms at z &gt; 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 &gt; 1, similar to that in the local Universe.

The Astrophysical Journal LettersVol. 979(2)
Damien Foundation (BD), Technical University of Denmark (DK)
National Science Foundation, Space Telescope Science Institute, National Research Foundation, Agence Nationale de la Recherche, Ministry of Education, Culture, Sports, Science and Technology, Danmarks Grundforskningsfond, National Natural Science Foundation of China, Centre National d’Etudes Spatiales, Japan Society for the Promotion of Science
Openalex Percentile: Top 13%
Galaxies: Formation, Evolution, Phenomena
2.31
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.