activity
20092026
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 17.2k across the 118 of their papers we have counts for

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8 papers · 1 filter

astro-ph.HE2022★ 19 cited

Effective resistivity in relativistic collisionless plasmoid-mediated reconnection

Sebastiaan Selvi, Oliver Porth, Bart Ripperda +3

Magnetic reconnection can power spectacular high-energy astrophysical phenomena by producing non-thermal energy distributions in highly magnetized regions around compact objects. B…

astro-ph.HE2022★ 40 cited

Radiation Transport Two-Temperature GRMHD Simulations of Warped Accretion Disks

M. T. P. Liska, N. Kaaz, G. Musoke +2

In many black hole systems, the accretion disk is expected to be misaligned with respect to the black hole spin axis. If the scale height of the disk is much smaller than the misal…

astro-ph.HE2022★ 38 cited

Nozzle Shocks, Disk Tearing and Streamers Drive Rapid Accretion in 3D GRMHD Simulations of Warped Thin Disks

Nicholas Kaaz, Matthew T. P. Liska, Jonatan Jacquemin-Ide +4

The angular momentum of gas feeding a black hole (BH) is typically misaligned with respect to the BH spin, resulting in a tilted accretion disk. Rotation of the BH drags the surrou…

astro-ph.HE2022★ 47 cited

Resolving the inner parsec of the blazar J1924-2914 with the Event Horizon Telescope

Sara Issaoun, Maciek Wielgus, Svetlana Jorstad +27

The blazar J1924-2914 is a primary Event Horizon Telescope (EHT) calibrator for the Galactic Center's black hole Sagittarius A*. Here we present the first total and linearly polari…

astro-ph.HE2022★ 112 cited

Millimeter light curves of Sagittarius A* observed during the 2017 Event Horizon Telescope campaign

Maciek Wielgus, Nicola Marchili, Ivan Marti-Vidal +28

The Event Horizon Telescope (EHT) observed the compact radio source, Sagittarius A* (Sgr A*), in the Galactic Center on 2017 April 5-11 in the 1.3 millimeter wavelength band. At th…

astro-ph.HE2022★ 37 cited

GRMHD Simulations of Accreting Neutron Stars with Non-Dipole Fields

Pushpita Das, Oliver Porth, Anna Watts

NASA's NICER telescope has recently provided evidence for non-dipolar magnetic field structures in rotation-powered millisecond pulsars. These stars are assumed to have gone throug…

astro-ph.HE2022★ 36 cited

Disk Tearing Leads to Low and High Frequency Quasi Periodic Oscillations in a GRMHD Simulation of a Thin Accretion Disk

G. Musoke, M. Liska, O. Porth +2

Black hole X-ray binaries (BHXRBs) display a wide range of variability phenomena, from long duration spectral state changes to short-term broadband variability and quasi-periodic o…

astro-ph.HE2022★ 99 cited

Formation of Magnetically Truncated Accretion Disks in 3D Radiation-Transport Two-Temperature GRMHD Simulations

M. T. P. Liska, G. Musoke, A. Tchekhovskoy +2

Multi-wavelength observations suggest that the accretion disk in the hard and intermediate states of X-ray binaries (XRBs) and active galactic nuclei (AGN) transitions from a cold,…