Coevolution (or not) of supermassive black holes and host galaxies

J Kormendy, LC Ho - Annual Review of Astronomy and …, 2013 - annualreviews.org
Supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …

Inward Bound---The Search For Supermassive Black Holes In Galactic Nuclei

J Kormendy, D Richstone - Annual Review of Astronomy and …, 1995 - adsabs.harvard.edu
Dynamical searches reveal central dark objects with masses $\sim 10^ 6$ to $10^{9.5}
$\msun in the Galaxy,\m31,\mm32, M87, NGC 3115, NGC 3377, NGC 4258, and NGC 4594 …

The Milky Way's bright satellites as an apparent failure of ΛCDM

M Boylan-Kolchin, JS Bullock… - Monthly Notices of the …, 2012 - academic.oup.com
We use the Aquarius simulations to show that the most massive subhaloes in galaxy-mass
dark matter (DM) haloes in Λ cold dark matter (ΛCDM) are grossly inconsistent with the …

The demography of massive dark objects in galaxy centers

J Magorrian, S Tremaine, D Richstone… - The Astronomical …, 1998 - iopscience.iop.org
We construct dynamical models for a sample of 36 nearby galaxies with Hubble Space
Telescope (HST) photometry and ground-based kinematics. The models assume that each …

The SAURON project—IV. The mass-to-light ratio, the virial mass estimator and the Fundamental Plane of elliptical and lenticular galaxies

M Cappellari, R Bacon, M Bureau… - Monthly Notices of …, 2006 - academic.oup.com
We investigate the well-known correlations between the dynamical mass-to-light ratio (M/L)
and other global observables of elliptical (E) and lenticular (S0) galaxies. We construct two …

SKIRT: An advanced dust radiative transfer code with a user-friendly architecture

P Camps, M Baes - Astronomy and Computing, 2015 - Elsevier
We discuss the architecture and design principles that underpin the latest version of SKIRT,
a state-of-the-art open source code for simulating continuum radiation transfer in dusty …

Analytical models for galactic nuclei

HS Zhao - Monthly Notices of the Royal Astronomical Society, 1996 - academic.oup.com
I present a general family of dynamical models with simple analytical potential-density pairs
suited to modelling galactic bulges and nuclei with double power-law radial density profiles …

Formation of galactic nuclei

M Milosavljević, D Merritt - The Astrophysical Journal, 2001 - iopscience.iop.org
We investigate a model in which galactic nuclei form via the coalescence of preexisting
stellar systems containing supermassive black holes. Merger simulations are carried out …

Measuring the inclination and mass-to-light ratio of axisymmetric galaxies via anisotropic Jeans models of stellar kinematics

M Cappellari - Monthly Notices of the Royal Astronomical …, 2008 - academic.oup.com
We present a simple and efficient anisotropic generalization of the semi-isotropic (two-
integral) axisymmetric Jeans formalism, which is used to model the stellar kinematics of …

Formation rate of extreme mass ratio inspirals in active galactic nuclei

Z Pan, H Yang - Physical Review D, 2021 - APS
Extreme mass ratio inspirals (EMRIs) are important sources for space-borne gravitational
wave detectors, such as the laser interferometer space antenna and TianQin. Previous EMRI …