Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations

  • Authors: Ruxin Barré, Arif Babul, Ghassem Gozaliasl, Alexis Finoguenov, Romeel Davé, Aviv Padawer-Blatt, Douglas Rennehan, Vida Saeedzadeh, Renier T. Hough, Thomas R. Quinn

Ruxin Barré et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 8.

BGG stellar age scaling relations. The BGG mass-weighted stellar age (Agew) is shown as a function of stellar mass in the top panel, and as a function of sSFR in the bottom panel. All formatting follows that of Figure 2. The vertical black line in the bottom panel represents the measurable ﹩\mathrm{log}({\rm{sSFR}}/{{\rm{yr}}}^{-1})﹩ > −12 limit.

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
Copyright and Terms & Conditions

Additional terms of reuse