In 14 simulated field dwarf galaxies, gas rotational support anti-correlates with the cumulative mass fraction accreted through mergers, indicating that assembly history rather than halo mass alone shapes dwarf galaxy kinematics.
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CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
In 14 simulated field dwarf galaxies, gas rotational support anti-correlates with the cumulative mass fraction accreted through mergers, indicating that assembly history rather than halo mass alone shapes dwarf galaxy kinematics.