The Black Hole Mass–Color Relations for Early- and Late-type Galaxies: Red and Blue Sequences

@article{Dullo2020TheBH,
title={The Black Hole Mass–Color Relations for Early- and Late-type Galaxies: Red and Blue Sequences},
author={B. T. Dullo and A. Bouquin and A. G. de Paz and J. Knapen and J. Gorgas},
journal={arXiv: Astrophysics of Galaxies},
year={2020}
}
[Abridged] Tight correlations between supermassive black hole (SMBH) mass ($M_{\rm BH}$) and the properties of the host galaxy have useful implications for our understanding of the growth of SMBHs and evolution of galaxies. Here, we present newly observed correlations between $M_{\rm BH}$ and the host galaxy total UV$-$ [3.6] color ($\mathcal{C_{\rm UV,tot}}$, Pearson's r = $0.6-0.7$) for a sample of 67 galaxies (20 early-type galaxies and 47 late-type galaxies) with directly measured $M_{\rm… Expand 2 Citations Figures and Tables from this paper Defining the (Black Hole)–Spheroid Connection with the Discovery of Morphology-dependent Substructure in the M BH–n sph and M BH–R e,sph Diagrams: New Tests for Advanced Theories and Realistic Simulations • Physics • 2020 For 123 local galaxies with directly-measured black hole masses (MBH), we provide the host spheroid’s Sérsic index (nsph), effective half-light radius (Re,sph), and effective surface brightness (μe),Expand BAYES-LOSVD: A Bayesian framework for non-parametric extraction of the line-of-sight velocity distribution of galaxies • Physics • 2020 We introduce BAYES-LOSVD, a novel implementation of the non-parametric extraction of line-of-sight velocity distributions (LOSVDs) in galaxies. We employ bayesian inference to obtain robust LOSVDsExpand References SHOWING 1-10 OF 251 REFERENCES Black Hole Mass Scaling Relations for Early-Type Galaxies:$M_{BH}$-$M_{*,sph}$and$M_{BH}$-$M_{*,gal}$• Physics • 2019 Analyzing a sample of 84 early-type galaxies with directly-measured super-massive black hole masses---nearly doubling the sample size of such galaxies with multi-component decompositions---aExpand Black Hole Mass Scaling Relations for Spiral Galaxies. II.$M_{\rm BH}$-$M_{\rm *,tot}$and$M_{\rm BH}$-$M_{\rm *,disk}$• Physics • 2018 Black hole mass ($M_{BH}$) scaling relations are typically derived using the properties of a galaxy's bulge and samples dominated by (high-mass) early-type galaxies. Studying late-type galaxiesExpand Updating the (Supermassive Black Hole Mass) - (Spiral Arm Pitch Angle) Relation: A Strong Correlation for Galaxies with Pseudobulges • Physics • 2017 We have conducted an image analysis of the (current) full sample of 44 spiral galaxies with directly measured supermassive black hole (SMBH) masses,$M_{\rm BH}$, to determine each galaxy'sExpand SUPERMASSIVE BLACK HOLES and THEIR HOST SPHEROIDS. II. the RED and BLUE SEQUENCE in the MBH-M∗,SPH DIAGRAM • Physics • 2016 In our first paper, we performed a detailed (i.e. bulge, disks, bars, spiral arms, rings, halo, nucleus, etc.) decomposition of 66 galaxies, with directly measured black hole masses,$M_{BH}$, thatExpand Galaxy And Mass Assembly (GAMA): Understanding the wavelength dependence of galaxy structure with bulge-disc decompositions With a large sample of bright, low-redshift galaxies with optical–near-IR imaging from the GAMA survey we use bulge-disc decompositions to understand the wavelength-dependent behaviour ofExpand The SINFONI Black Hole Survey: The Black Hole Fundamental Plane revisited and the paths of (co-) evolution of supermassive black holes and bulges We investigate the correlations between the black hole mass$M_{BH}$, the velocity dispersion$\sigma$, the bulge mass$M_{Bu}$, the bulge average spherical density$\rho_h$and its spherical halfExpand Improved Dynamical Constraints on the Masses of the Central Black Holes in Nearby Low-mass Early-type Galactic Nuclei And the First Black Hole Determination for NGC 205 We improve the dynamical black hole (BH) mass estimates in three nearby low-mass early-type galaxies--NGC 205, NGC 5102, and NGC 5206. We use new \hst/STIS spectroscopy to fit the star formationExpand How Mergers May Affect the Mass Scaling Relation between Gravitationally Bound Systems Supermassive black hole (BH) masses ($m{c M}BH$-->$m{c M}t SUBgt BHt/SUBgt $-->) are strongly correlated with galaxy stellar bulge masses ($m{c M}bulge$-->$m{c M}t SUBgt bulget/SUBgt \$ -->), andExpand
Two channels of supermassive black hole growth as seen on the galaxies mass–size plane
• Physics
• 2017
We investigate the variation of black hole masses (Mbh) as a function of their host galaxy stellar mass (Mstar) and half-light radius (Re). We confirm that the scatter in Mbh within this plane isExpand