Preprint
Supermassive black hole pairs in clumpy galaxies at high redshift: delayed binary formation and concurrent mass growth
Abstract
Massive gas-rich galaxy discs at $z \sim 1-3$ host massive star-forming
clumps with typical baryonic masses in the range $10^7-10^8$~M$_{\odot}$ which
Authors
Tamburello V; Capelo PR; Mayer L; Bellovary JM; Wadsley J
Publication date
February 29, 2016
DOI
10.48550/arxiv.1603.00021
Preprint server
arXiv