The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes - CNRS - Centre national de la recherche scientifique Accéder directement au contenu
Article Dans Une Revue Monthly Notices of the Royal Astronomical Society Année : 2020

The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes

Katarina Kraljic
Christophe Pichon
Sandrine Codis
Romeel Davé
  • Fonction : Auteur
Yohan Dubois
Ho Seong Hwang
Dmitri Pogosyan
  • Fonction : Auteur
Julien Devriendt
Marcello Musso
  • Fonction : Auteur
Adrianne Slyz
  • Fonction : Auteur

Résumé

We investigate the impact of the number of filaments connected to the nodes of the cosmic web on the physical properties of their galaxies using the Sloan Digital Sky Survey. We compare these measurements to the cosmological hydrodynamical simulations H orizon-(no)AGN and Simba. We find that more massive galaxies are more connected, in qualitative agreement with theoretical predictions and measurements in dark-matter-only simulations. The star formation activity and morphology of observed galaxies both display some dependence on the connectivity of the cosmic web at a fixed stellar mass: Less star forming and less rotation supported galaxies also tend to have higher connectivity. These results qualitatively hold both for observed and for virtual galaxies, and can be understood given that the cosmic web is the main source of fuel for galaxy growth. The simulations show the same trends at a fixed halo mass, suggesting that the geometry of filamentary infall impacts galaxy properties beyond the depth of the local potential well. Based on simulations, it is also found that active galactic nucleus feedback is key to reversing the relationship between stellar mass and connectivity at a fixed halo mass. Technically, connectivity is a practical observational proxy for past and present accretion (minor mergers or diffuse infall).
Fichier principal
Vignette du fichier
stz3319.pdf (3.47 Mo) Télécharger le fichier
Origine : Fichiers éditeurs autorisés sur une archive ouverte

Dates et versions

hal-02423677 , version 1 (26-08-2022)

Identifiants

Citer

Katarina Kraljic, Christophe Pichon, Sandrine Codis, Clotilde Laigle, Romeel Davé, et al.. The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes. Monthly Notices of the Royal Astronomical Society, 2020, 491 (3), pp.4294-4309. ⟨10.1093/mnras/stz3319⟩. ⟨hal-02423677⟩
142 Consultations
36 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More