Rayleigh–Taylor and Richtmyer–Meshkov instability induced flow, turbulence, and mixing. II
Y Zhou - Physics Reports, 2017 - Elsevier
Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …
pathways towards turbulent mixing layers, in many cases characterized by significant mass …
The origin of radio emission from radio-quiet active galactic nuclei
The central nuclei of galaxies, where supermassive black holes (SMBHs) are thought to
reside, can experience phases of activity when they become active galactic nuclei (AGNs) …
reside, can experience phases of activity when they become active galactic nuclei (AGNs) …
[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 …
[HTML][HTML] First Sagittarius A* event horizon telescope results. V. Testing astrophysical models of the galactic center black hole
In this paper we provide a first physical interpretation for the Event Horizon Telescopeʼs
(EHT) 2017 observations of Sgr A*. Our main approach is to compare resolved EHT data at …
(EHT) 2017 observations of Sgr A*. Our main approach is to compare resolved EHT data at …
[HTML][HTML] First Sagittarius A* event horizon telescope results. II. EHT and multiwavelength observations, data processing, and calibration
Abstract We present Event Horizon Telescope (EHT) 1.3 mm measurements of the radio
source located at the position of the supermassive black hole Sagittarius A*(Sgr A*) …
source located at the position of the supermassive black hole Sagittarius A*(Sgr A*) …
[HTML][HTML] First M87 event horizon telescope results. VIII. Magnetic field structure near the event horizon
Abstract Event Horizon Telescope (EHT) observations at 230GHz have now imaged
polarized emission around the supermassive black hole in M87 on event-horizon scales …
polarized emission around the supermassive black hole in M87 on event-horizon scales …
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 …
Orbital motion near Sagittarius A*-Constraints from polarimetric ALMA observations
We report on the polarized light curves of the Galactic Center supermassive black hole
Sagittarius A*, obtained at millimeter wavelength with the Atacama Large Millimeter …
Sagittarius A*, obtained at millimeter wavelength with the Atacama Large Millimeter …
First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multi-wavelength Observations, Data Processing, and Calibration
Event Horizon Telescope Collaboration - arXiv preprint arXiv …, 2023 - arxiv.org
We present Event Horizon Telescope (EHT) 1.3 mm measurements of the radio source
located at the position of the supermassive black hole Sagittarius A*(Sgr A*), collected …
located at the position of the supermassive black hole Sagittarius A*(Sgr A*), collected …
Polarimetry and astrometry of NIR flares as event horizon scale, dynamical probes for the mass of Sgr A
We present new astrometric and polarimetric observations of flares from Sgr A* obtained
with GRAVITY, the near-infrared interferometer at ESO's Very Large Telescope …
with GRAVITY, the near-infrared interferometer at ESO's Very Large Telescope …