The Hydrostatic Mass of A478: Discrepant Results From Chandra, NuSTAR, and XMM-Newton

Galaxy clusters are the most recently formed and most massive, gravitationally bound structures in the universe. The number of galaxy clusters formed is highly dependent on cosmological parameters, such as the dark matter density, $\sigma_8$, and $\Omega_m$. The number density is a function of the c...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Potter, Cicely, Tümer, Ayşegül, Wang, Qian H. S, Wik, Daniel R, Maughan, Ben J, Schellenberger, Gerrit
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!