Importance of Initial Condition on Bar Secular Evolution: Role of Halo Angular Momentum Discontinuity|Simulation Data
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This data includes the key snapshots of the simulations in GADGAET-2 format. The folders, namely D0, D1, D2, and D3, correspond to the four galaxy models used in this study. The snapshots are printed from time=0 Gyr to 10Gyr in a timestep of 1 Gyr.
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2023-05-24



