Study of galaxies on large-scale filaments in simulations
ABSTRACT We use data from the Evolution and Assembly of GaLaxies in their Environment (eagle) cosmological simulation to study properties of galaxies in the cosmic web. Galaxies become more redder and form stars at a lower rate relative to their counterparts further away from the cylindrical axis of...
Gespeichert in:
| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2020-09, Vol.497 (2), p.2265-2275 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| Zusammenfassung: | ABSTRACT
We use data from the Evolution and Assembly of GaLaxies in their Environment (eagle) cosmological simulation to study properties of galaxies in the cosmic web. Galaxies become more redder and form stars at a lower rate relative to their counterparts further away from the cylindrical axis of the large-scale filaments. These trends are particularly strong for galaxies with M*/M⊙ ≲ 1010. We also find that at distances |
|---|---|
| ISSN: | 0035-8711 1365-2966 |
| DOI: | 10.1093/mnras/staa1913 |