The orbital geometry of a galaxy merger, spiral-in versus direct collision, systematically controls the disk, bulge, and hot halo fractions of the remnant galaxy in IllustrisTNG-100.
D., Naab, T., & Scannapieco, C
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The effects of the orbital configurations of mergers on reshaping galaxy structures
The orbital geometry of a galaxy merger, spiral-in versus direct collision, systematically controls the disk, bulge, and hot halo fractions of the remnant galaxy in IllustrisTNG-100.