Maximum black hole mass across cosmic time

ABSTRACT At the end of its life, a very massive star is expected to collapse into a black hole (BH). The recent detection of an 85  M⊙ BH from the gravitational wave event GW 190521 appears to present a fundamental problem as to how such heavy BHs exist above the approximately 50  M⊙ pair-instabilit...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2021-06, Vol.504 (1), p.146-154
Hauptverfasser:	Vink, Jorick S, Higgins, Erin R, Sander, Andreas A C, Sabhahit, Gautham N
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!