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 …
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …
The Galactic Center massive black hole and nuclear star cluster
R Genzel, F Eisenhauer, S Gillessen - Reviews of modern physics, 2010 - APS
The Galactic Center is an excellent laboratory for studying phenomena and physical
processes that may be occurring in many other galactic nuclei. The center of our Milky Way …
processes that may be occurring in many other galactic nuclei. The center of our Milky Way …
[HTML][HTML] First Sagittarius A* event horizon telescope results. VI. Testing the black hole metric
Astrophysical black holes are expected to be described by the Kerr metric. This is the only
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
Event Horizon Telescope Collaboration - arXiv preprint arXiv …, 2023 - arxiv.org
Astrophysical black holes are expected to be described by the Kerr metric. This is the only
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
Relativistic redshift of the star S0-2 orbiting the Galactic Center supermassive black hole
The general theory of relativity predicts that a star passing close to a supermassive black
hole should exhibit a relativistic redshift. In this study, we used observations of the Galactic …
hole should exhibit a relativistic redshift. In this study, we used observations of the Galactic …
An update on monitoring stellar orbits in the galactic center
S Gillessen, PM Plewa, F Eisenhauer… - The Astrophysical …, 2017 - iopscience.iop.org
Using 25 years of data from uninterrupted monitoring of stellar orbits in the Galactic Center,
we present an update of the main results from this unique data set: a measurement of mass …
we present an update of the main results from this unique data set: a measurement of mass …
An improved distance and mass estimate for Sgr A* from a multistar orbit analysis
A Boehle, AM Ghez, R Schödel, L Meyer… - The Astrophysical …, 2016 - iopscience.iop.org
We present new, more precise measurements of the mass and distance of our Galaxy's
central supermassive black hole, Sgr A*. These results stem from a new analysis that more …
central supermassive black hole, Sgr A*. These results stem from a new analysis that more …
Probing Lorentz symmetry violation using the first image of Sagittarius A*: Constraints on standard-model extension coefficients
M Khodadi, G Lambiase - Physical Review D, 2022 - APS
Thanks to unparalleled near-horizon images of the shadows of Messier 87*(M87*) and
Sagittarius A*(Sgr A*) delivered by the Event Horizon Telescope (EHT), two amazing …
Sagittarius A*(Sgr A*) delivered by the Event Horizon Telescope (EHT), two amazing …
[图书][B] Galaxy formation and evolution
The rapidly expanding field of galaxy formation lies at the interface between astronomy,
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …
Formation of supermassive black holes
M Volonteri - The Astronomy and Astrophysics Review, 2010 - Springer
Evidence shows that massive black holes reside in most local galaxies. Studies have also
established a number of relations between the MBH mass and properties of the host galaxy …
established a number of relations between the MBH mass and properties of the host galaxy …