The fundamental relation between supermassive black holes and their host galaxies. Issue 1 (5th September 2019)

• Record Type: Journal Article
• Authors: de Nicola, Stefano; Marconi, Alessandro; Longo, Giuseppe
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 490:Issue 1(2019)
• Page Start: 600
• Page End: 612
• Publication Date: 2019-09-05
• Subjects: Galaxy: fundamental parameters; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz2472
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We study the correlations between supermassive black holes (BHs) and their host galaxies, using a sample of 83 BH masses collected from the most recent and reliable spatially resolved estimates available from the literature. We confirm the mono- and bivariate correlations between SMBHs and the bulges of their host galaxies, confirming that the correlation with the effective velocity dispersion is not significantly improved by higher dimensionality. Instead, pseudo-bulges do not seem to correlate with their SMBHs, probably because their secular evolution is often unable to trigger accretion onto the central BH. We then present a novel approach aimed at finding the fundamental relation between SMBHs and their host galaxies. For the first time, we analytically combine BH masses with the Fundamental Plane (FP), showing that M BH –σ e appears to be the fundamental relation rather than a putative 'BH Fundamental Plane' of the kind M BH –σ e – Re . These results can be explained by a picture which sees the M BH –σ e relation as a natural outcome of the change in AGN feedback from momentum-driven to energy-driven. The other scaling relations are then established through the FP.