An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
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Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing bandObserving the Galaxy's massive black hole with gravitational wave burstsMeasuring the Masses of Supermassive Black HolesKinematics and excitation of the molecular hydrogen accretion disc in NGC 1275The overmassive black hole in NGC 1277: new constraints from molecular gas kinematicsWhat produces the extended LINER-type emission in the NUGA galaxy NGC 5850?Search for intermediate mass black hole binaries in the first observing run of Advanced LIGOAre Nuclear Star Clusters the Precursors of Massive Black Holes?The Low-Mass End of theMBH/MhostRelation in QuasarsA Practical Guide to the Massive Black Hole Cosmic HistoryMassive Black Hole Binaries: Dynamical Evolution and Observational SignaturesMass Functions of Supermassive Black Holes across Cosmic TimeBAT AGN Spectroscopic Survey – III. An observed link between AGN Eddington ratio and narrow-emission-line ratiosThe spectral energy distributions, host galaxies and environments of variability-selected active galactic nuclei in GOODS-SouthFaint high-redshift AGN in theChandradeep field south: the evolution of the AGN luminosity function and black hole demographyEnhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observationsGalaxy Zoo: the effect of bar-driven fuelling on the presence of an active galactic nucleus in disc galaxiesThe most massive black holes on the Fundamental Plane of black hole accretionBlack hole growth to z = 2 - I. Improved virial methods for measuring MBH and L/LEddExtending virial black hole mass estimates to low-luminosity or obscured AGN: the cases of NGC 4395 and MCG -01-24-012B2 0954+25A: a typical Fermi blazar or a γ-ray loud Narrow Line Seyfert 1≟Detection of faint broad emission lines in type 2 AGNs – III. On the MBH-σ⋆ relation of type 2 AGNsRelative growth of black holes and the stellar components of galaxiesZFOURGE catalogue of AGN candidates: an enhancement of 160-μm-derived star formation rates in active galaxies toz = 3.2
P2860
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P2860
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
description
im Januar 2011 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в січні 2011
@uk
name
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
@en
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
@nl
type
label
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
@en
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
@nl
prefLabel
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
@en
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
@nl
P2093
P2860
P1476
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses
@en
P2093
Alister W. Graham
Christopher A. Onken
E. Athanassoula
P2860
P304
P356
10.1111/J.1365-2966.2010.18045.X
P407
P577
2011-01-18T00:00:00Z
P818
P819
2011MNRAS.412.2211G