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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 9.

Galaxies in stellar mass-size space at different redshifts, colored by the median nearest filament density (top row) and the median stellar sAM (bottom row). The dashed and dotted curves correspond to the median relationship and 25th and 75th percentiles, respectively. More extended galaxies typically have higher spin and at z ≥ 0.5 live in higher-density filaments.

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