The Fundamental Signature of Star Formation Quenching from AGN Feedback: A Critical Dependence of Quiescence on Supermassive Black Hole Mass, Not Accretion Rate (2023)

First Author: Bluck A
Attributed to:  Support of the Astronomical Research of the Cavendish Astrophysics Group funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.17863/cam.94187

Publication URI: https://www.repository.cam.ac.uk/handle/1810/346772

Type: Journal Article/Review