TNG50 simulations show the fraction and amplitude of lopsided disk galaxies decrease from about 60% at redshift 2 to about 40% today, with interactions and gas accretion more effective at high redshift.
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Tracing the origins of galaxy lopsidedness across cosmic time
TNG50 simulations show the fraction and amplitude of lopsided disk galaxies decrease from about 60% at redshift 2 to about 40% today, with interactions and gas accretion more effective at high redshift.