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Discovery of Very Minor Merger-Induced Star-forming Clumps at $z=3.33$ with JWST
High-redshift galaxies often contain ''clumps:'' compact, $\sim$kpc-scale regions of intense star formation. These substructures make up significant fractions of the masses and star-formation rates of their host galaxies and are expected to affect the morphologies of their hosts, such as by building
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