Spiral arms in z~1.5 galaxies show optical-to-near-infrared flux peak offsets of 0.2 to 0.8 kpc, consistent with density waves, tidal interactions, and clumpy star formation as seen locally.
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A multi-wavelength investigation of spiral structures in $z > 1$ galaxies with JWST
Spiral arms in z~1.5 galaxies show optical-to-near-infrared flux peak offsets of 0.2 to 0.8 kpc, consistent with density waves, tidal interactions, and clumpy star formation as seen locally.