Quenching massive galaxies across cosmic time with the semi-analytic model SHARK v2.0

We introduce version 2.0 of the SHARK semi-analytic model of galaxy formation after many improvements to the physics included. The most significant being: (i) a model describing the exchange of angular momentum (AM) between the interstellar medium and stars; (ii) a new active galactic nuclei feedbac...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2024-04
Hauptverfasser:	Lagos, Claudia D P, Bravo, Matias, Tobar, Rodrigo, Obreschkow, Danail, Power, Chris, Robotham, Aaron S G, Proctor, Katy L, Hansen, Samuel, Chandro-Gomez, Angel, Carrivick, Julian
Format:	Artikel
Sprache:	eng
Schlagworte:	Accuracy Active galactic nuclei Angular momentum Environment models Environmental effects Galactic evolution Galaxies Interstellar matter Mathematical models Particle swarm optimization Quasars Quenching Sharks Star & galaxy formation Star formation rate Stellar mass
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!