Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 8.

The residual effect of filament density on stellar kinematic morphological properties at fixed mass. The three panels show the residual stellar sAM (left), fraction of stars with disk orbits (middle), and fraction of stars with bulge orbits (right). The much larger vertical range for the left panel reflects the much stronger residual dependence of stellar sAM on the filament density. The bulge and disk fractions have a smaller residual dependence on the filament density.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse