Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations

  • Authors: Hassen M. Yesuf, Connor Bottrell, Luis C. Ho, Aaron S. G. Robotham, Sabine Bellstedt, Robin H. W. Cook, Lei Hao, Fengshan Liu

Hassen M. Yesuf et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure A3.

Outer asymmetry function. Number densities of galaxies as a function of i-band outer asymmetry are shown in panels for three stellar mass bins (﹩{\rm{log}}({M}_{\star }/{M}_{\odot })=10.0﹩–10.5, 10.5–11.0, 11.0–11.5) and three star formation categories (all galaxies, star-forming: ﹩{\rm{\Delta }}\mathrm{log}{\rm{SFR}}\gt -1﹩, quiescent: ﹩{\rm{\Delta }}\mathrm{log}{\rm{SFR}}\lt -1﹩).

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