Answers are grounded in this paper and cite their sources.
Aims. We explore the connection between black hole growth at the center of obscured quasars selected from the XMM-COSMOS survey and the physical properties of their host galaxies. We study a bolometric regime ( ⟨ Lbol ⟩ = 8 × 1045 erg s-1) where several theoretical models invoke major galaxy mergers as the main fueling channel for black hole accretion.
No takes yet. Share an insight, caveat, or question.
A 2011 study studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: