First Very Long Baseline Interferometry Detections at 870μm
First Sagittarius A* Event Horizon Telescope Results: VII. Polarization of the Ring
Ordered Magnetic Fields Around the 3C 84 Central Black Hole
On the Comparison of AGN with GRMHD Simulations: II. M87
A search for pulsars around Sgr A* in the first Event Horizon Telescope dataset
First M87 Event Horizon Telescope Results. IX: Detection of Near-Horizon Circular Polarization
Polarimetric Geometric Modeling for mm-VLBI Observations of Black Holes
Comparison of Polarized Radiative Transfer Codes used by the EHT Collaboration
Accreting Primordial Black Holes and Dark Matter Candidates
The Event Horizon Telescope Image of the Quasar NRAO 530
Modeling Reconstructed Images of Jets Launched by SANE Super-Eddington Accretion Flows Around SMBHs with the ngEHT (v1) (v2)
Probing Plasma Composition with the Next Generation Event Horizon Telescope (ngEHT) (v1) (v2)
Tracing the Hotspot Motion Using the Next Generation Event Horizon Telescope (ngEHT) (v1) (v2)
Emission Modeling in the EHT-ngEHT Age (v1) (v2)
Unraveling Twisty Linear Polarization Morphologies in Black Hole Images (v1) (v2)
Jets from SANE Super-Eddington Accretion Disks: Morphology, Spectra and Their Potential as Targets for ngEHT (v1) (v2)
First Sagittarius A* Event Horizon Telescope Results. VI. Testing the Black Hole Metric
Selective Dynamical Imaging of Interferometric Data
The Variability of the Black-Hole Image in M87 at the Dynamical Timescale
Millimeter Light Curves of Sgr A* Observed during the 2017 Event Horizon Telescope Campaign
Positron Effects on Polarized Images and Spectra from Jet and Accretion Flow Models of M87 and Sgr A* (v1) (v2) (v3) (v4)
Event Horizon Telescope observations of the jet launching and collimation in Centaurus A
Constraints on black-hole charges with the 2017 EHT observations of M87*
Broadband Multi-Wavelength Properties of M87 During the 2017 Event Horizon Telescope Campaign
First Event Horizon Telescope Results. VIII. Magnetic Field Structure Near the Event Horizon
First Event Horizon Telescope Results. VII. Polarization of the Ring
Polarimetric Properties of Event Horizon Telescope Targets from ALMA
On the Comparison of AGN with GRMHD Simulations. I: Sgr A* (v1) (v2)
Determining the Composition of Relativistic Jets from Polarization Maps (v1) (v2)
A Quasi-Static Hyper-Resistive Model of UHE Cosmic Ray Acceleration by Magnetically Collimated Jets Created by AGN (v1) (v2)
The Future of Black Hole Astrophysics in the LIGO-VIRGO-LPF Era
The Pauli Exclusion Principle at Strong Coupling – Holographic Matter and Momentum Space
TeV gamma rays from distant BL-Lacs and photon-paraphoton kinetic mixing
Grand Unification Scale Primordial Black Holes – Consequences and Constraints
Cover Story (view full-size image) M87 jet magnetic flux tubes are observed here at 15 GHz by the VLBA (courtesy of Kellermann, K.; et al.), possibly indicative of the magnetic Kelvin-Helmholtz instability. This pattern also appears in simulation models (Anantua et al. 2018) when the energy density of relativistic electrons in the radio jet does not decline with magnetic field strength at increasing radii from the black hole. With observation length scales over an order of magnitude greater than simulation scales, more remote processes such as coupling to the rotating interstellar medium may be responsible for the twisting flux tubes observed than in the simulation. Finite VLBA imaging resolution may restrict observers to seeing only the largest structures (the m = ±1 modes), while it may be possible to resolve smaller-scale structure in simulations. With the “Observing” Jet/Accretion Disk/Black Hole (JAB) simulations methodology, we may analyze disk/jet magnetohydrodynamic interactions to be exhibited by the EHT.