The same major merger produces compact disk remnants in codes with kinetic feedback, late disks in thermal-only codes, and no disk in delayed-cooling/superbubble codes, with the remnant disk always aligned to the merger orbit.
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The AGORA High-resolution Galaxy Simulations Comparison Project. IX - Part 2: Effects of a Major Galaxy Merger on the Stellar Morphology of a Milky Way-mass Galaxy Progenitor
The same major merger produces compact disk remnants in codes with kinetic feedback, late disks in thermal-only codes, and no disk in delayed-cooling/superbubble codes, with the remnant disk always aligned to the merger orbit.