On the black hole mass-bulge mass relation
N. Häring,Hans-Walter Rix +1 more
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In this paper, the authors examined the relation between the mass of the central black holes in nearby galaxies, Mbh, and the stellar mass of surrounding spheroid or bulge, Mbulge.Abstract:
We have reexamined the relation between the mass of the central black holes in nearby galaxies, Mbh, and the stellar mass of the surrounding spheroid or bulge, Mbulge. For a total of 30 galaxies bulge masses were derived through Jeans equation modeling or adopted from dynamical models in the literature. In stellar mass-to-light ratios, the spheroids and bulges span a range of a factor of 8. The bulge masses were related to well-determined black hole masses taken from the literature. With these improved values for Mbh, compared to Magorrian et al., and our redetermination of Mbulge, we find that the Mbh-Mbulge relation becomes very tight. We find Mbh ~ M with an observed scatter of 0.30 dex, a fraction of which can be attributed to measurement errors. The scatter in this relation is therefore comparable to the scatter in the relations of Mbh with σ and the stellar concentration. These results confirm and refine the work of Marconi & Hunt. For Mbulge ~ 5 × 1010 M☉ the median black hole mass is 0.14% ± 0.04% of the bulge mass.read more
Citations
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Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
John Kormendy,Luis C. Ho +1 more
TL;DR: In this paper, supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of spatially resolved kinematics, and it has been shown that BHs and bulges coevolve by regulating each other's growth.
Journal ArticleDOI
Breaking the hierarchy of galaxy formation
Richard G. Bower,Andrew J. Benson,Rowena K. Malbon,John C. Helly,Carlos S. Frenk,Carlton M. Baugh,Shaun Cole,Cedric G. Lacey +7 more
TL;DR: In this paper, a new implementation of the Durham semi-analytic model of galaxy formation in which feedback due to active galactic nuclei (AGN) is assumed to quench cooling flows in massive halos is discussed.
Journal ArticleDOI
Observational Evidence of Active Galactic Nuclei Feedback
TL;DR: In this article, it was shown that the radiative or quasar mode of feedback can account for the observed proportionality between the central black hole and the host galaxy mass, which can lead to ejection or heating of the gas.
Journal ArticleDOI
CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
Norman A. Grogin,Dale D. Kocevski,Sandra M. Faber,Henry C. Ferguson,Anton M. Koekemoer,Adam G. Riess,Viviana Acquaviva,David M. Alexander,Omar Almaini,Matthew L. N. Ashby,Marco Barden,Eric F. Bell,Frédéric Bournaud,Thomas M. Brown,Karina Caputi,Stefano Casertano,Paolo Cassata,Marco Castellano,Peter Challis,Ranga-Ram Chary,Edmond Cheung,Michele Cirasuolo,Christopher J. Conselice,Asantha Cooray,Darren J. Croton,Emanuele Daddi,Tomas Dahlen,Romeel Davé,Duilia F. de Mello,Duilia F. de Mello,Avishai Dekel,Mark Dickinson,Timothy Dolch,Jennifer L. Donley,James Dunlop,Aaron A. Dutton,David Elbaz,Giovanni G. Fazio,Alexei V. Filippenko,Steven L. Finkelstein,Adriano Fontana,Jonathan P. Gardner,Peter M. Garnavich,Eric Gawiser,Mauro Giavalisco,Andrea Grazian,Yicheng Guo,Nimish P. Hathi,Boris Häussler,Philip F. Hopkins,Jiasheng Huang,Kuang-Han Huang,Kuang-Han Huang,Saurabh Jha,Jeyhan S. Kartaltepe,Robert P. Kirshner,David C. Koo,Kamson Lai,Kyoung-Soo Lee,Weidong Li,Jennifer M. Lotz,Ray A. Lucas,Piero Madau,Patrick J. McCarthy,Elizabeth J. McGrath,Daniel H. McIntosh,Ross J. McLure,Bahram Mobasher,Leonidas A. Moustakas,Mark Mozena,Kirpal Nandra,Jeffrey A. Newman,Sami Niemi,Kai G. Noeske,Casey Papovich,Laura Pentericci,Alexandra Pope,Joel R. Primack,Abhijith Rajan,Swara Ravindranath,Naveen A. Reddy,Alvio Renzini,Hans-Walter Rix,Aday R. Robaina,Steven A. Rodney,David J. Rosario,Piero Rosati,S. Salimbeni,Claudia Scarlata,Brian Siana,Luc Simard,Joseph Smidt,Rachel S. Somerville,Hyron Spinrad,Amber Straughn,Louis-Gregory Strolger,Olivia Telford,Harry I. Teplitz,Jonathan R. Trump,Arjen van der Wel,Carolin Villforth,Risa H. Wechsler,Benjamin J. Weiner,Tommy Wiklind,Vivienne Wild,Grant W. Wilson,Stijn Wuyts,Hao Jing Yan,Min S. Yun +108 more
TL;DR: The Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS) as discussed by the authors was designed to document the first third of galactic evolution, from z approx. 8 - 1.5 to test their accuracy as standard candles for cosmology.
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The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
Darren J. Croton,Volker Springel,Simon D. M. White,G. De Lucia,Carlos S. Frenk,Liang Gao,Adrian Jenkins,Guinevere Kauffmann,Julio F. Navarro,Naoki Yoshida +9 more
TL;DR: In this article, the authors simulate the growth of galaxies and their central supermassive black holes by implementing a suite of semi-analytic models on the output of the Millennium Run, a very large simulation of the concordance A cold dark matter cosmogony.
References
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Book
An introduction to the bootstrap
Bradley Efron,Robert Tibshirani +1 more
TL;DR: This article presents bootstrap methods for estimation, using simple arguments, with Minitab macros for implementing these methods, as well as some examples of how these methods could be used for estimation purposes.
Journal ArticleDOI
An Introduction to the Bootstrap.
Book ChapterDOI
Third Reference Catalogue of Bright Galaxies
Gerard de Vaucouleurs,Antoinette de Vaucouleurs,Harold G. Corwin,Ronald J. Buta,G. Paturel,P. Fouque +5 more
TL;DR: In this article, a reference catalogue of bright galaxies in three volumes reflects the explosive growth of extragalactic astronomy over the last 15 years and includes all galaxies with apparent diameters larger than one arc minute, magnitudes brighter than about magnitude 15.5, and redshifts not larger than 15,000 km/sec.
Journal ArticleDOI
A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
TL;DR: The mass of supermassive black holes correlate almost perfectly with the velocity dispersions of their host bulges, Mbh ∝ σα, where α = 48 ± 05.