Group-scale halos produce a dual effect on infalling galaxies: pre-processing raises quiescent fraction early, while protection delays cluster-driven quenching to smaller d_R.
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Live halos with sufficient mass resolution enable cascading multi-mode spirals in galactic disks through swing amplification and mode interference, absent in fixed-potential or coarsely resolved models.
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The dual effect of group-scale environments on galaxy quenching during cluster infall: pre-processing and protection
Group-scale halos produce a dual effect on infalling galaxies: pre-processing raises quiescent fraction early, while protection delays cluster-driven quenching to smaller d_R.
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Effects of Resolution and Local Stability on Galactic Disks: I. Multiple Spiral Mode Formation via Swing Amplification
Live halos with sufficient mass resolution enable cascading multi-mode spirals in galactic disks through swing amplification and mode interference, absent in fixed-potential or coarsely resolved models.