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Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman

  • Authors: Farhanul Hasan, Haowen Zhang, 昊文 张, Viraj Pandya, Marc Rafelski, Joseph N. Burchett, Douglas Hellinger, Kalina V. Nedkova, Ilias Goovaerts, Nir Mandelker, Daisuke Nagai, Grecco A. Oyarzún, Joel R. Primack, Joanna Woo

Farhanul Hasan et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 5.

Fraction of prolate subhalos (color bar) as a function of filament line density (y-axis) and subhalo DM mass (x-axis) at different redshifts in TNG50-Dark. The top and bottom rows represent the shape measured within 0.1rDM (inner halo) and 2rDM (outer halo), respectively. In this DM-only simulation, higher-mass halos (especially inner halos) are more prolate.

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