Clumps in low-redshift analogues of high-redshift galaxies are a few hundred parsecs across, and simulated cosmic-noon observations show that clustering and limited resolution inflate their apparent sizes.
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Low-redshift analogues of cosmic noon galaxies as laboratories for clumpy star formation
Clumps in low-redshift analogues of high-redshift galaxies are a few hundred parsecs across, and simulated cosmic-noon observations show that clustering and limited resolution inflate their apparent sizes.