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19922023
most citedSpectra and Light Curves of Gamma-Ray Burst Afterglows

2.3k citations · 53.2k across the 308 of their papers we have counts for

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Showing 2021Show all

12 papers · 1 filter

physics.plasm-ph2021★ 1 cited

Building a weak shockwave from linear modes

Antoine Bret, Ramesh Narayan

In shockwave theory, the density, velocity and pressure jumps are derived from the conservation equations. Here, we address the physics of a weak shock the other way around. We fir…

astro-ph.GA2021★ 139 cited

Event Horizon Telescope observations of the jet launching and collimation in Centaurus A

Michael Janssen, Heino Falcke, Matthias Kadler +236

Very-long-baseline interferometry (VLBI) observations of active galactic nuclei at millimeter wavelengths have the power to reveal the launching and initial collimation region of e…

astro-ph.HE2021★ 18 cited

The Variability of the Black-Hole Image in M87 at the Dynamical Time Scale

Kaushik Satapathy, Dimitrios Psaltis, Feryal Ozel +235

The black-hole images obtained with the Event Horizon Telescope (EHT) are expected to be variable at the dynamical timescale near their horizons. For the black hole at the center o…

astro-ph.HE2021★ 63 cited

Faraday depolarization and induced circular polarization by multi-path propagation with application to FRBs

Paz Beniamini, Pawan Kumar, Ramesh Narayan

We describe how the observed polarization properties of an astronomical object are related to its intrinsic polarization properties and the finite temporal and spectral resolutions…

astro-ph.HE2021★ 171 cited

Jets in Magnetically Arrested Hot Accretion Flows: Geometry, Power and Black Hole Spindown

Ramesh Narayan, Andrew Chael, Koushik Chatterjee +2

We present the results of nine simulations of radiatively-inefficient magnetically arrested disks (MADs) across different values of the black hole spin parameter : , $-0…

astro-ph.HE2021★ 71 cited

Toward determining the number of observable supermassive black hole shadows

Dominic W. Pesce, Daniel C. M. Palumbo, Ramesh Narayan +7

We present estimates for the number of shadow-resolved supermassive black hole (SMBH) systems that can be detected using radio interferometers, as a function of angular resolution,…

gr-qc2021★ 350 cited

Constraints on black-hole charges with the 2017 EHT observations of M87*

Prashant Kocherlakota, Luciano Rezzolla, Heino Falcke +234

Our understanding of strong gravity near supermassive compact objects has recently improved thanks to the measurements made by the Event Horizon Telescope (EHT). We use here the M8…

astro-ph.HE2021★ 89 cited

The Polarized Image of a Synchrotron Emitting Ring of Gas Orbiting a Black Hole

Ramesh Narayan, Daniel C. M. Palumbo, Michael D. Johnson +237

Synchrotron radiation from hot gas near a black hole results in a polarized image. The image polarization is determined by effects including the orientation of the magnetic field i…

astro-ph.HE2021★ 25 cited

Brightness Asymmetry of Black Hole Images as a Probe of Observer Inclination

Lia Medeiros, Chi-Kwan Chan, Ramesh Narayan +2

The Event Horizon Telescope recently captured images of the supermassive black hole in the center of the M87 galaxy, which show a ring-like emission structure with the South side o…

astro-ph.GA2021★ 111 cited

Polarimetric properties of Event Horizon Telescope targets from ALMA

Ciriaco Goddi, Ivan Marti-Vidal, Hugo Messias +31

We present the results from a full polarization study carried out with ALMA during the first VLBI campaign, which was conducted in Apr 2017 in the 3mm and 1.3mm bands, in con…

astro-ph.HE2021★ 469 cited

First M87 Event Horizon Telescope Results. VII. Polarization of the Ring

The Event Horizon Telescope Collaboration

In 2017 April, the Event Horizon Telescope (EHT) observed the near-horizon region around the supermassive black hole at the core of the M87 galaxy. These 1.3 mm wavelength observat…

astro-ph.HE2021★ 44 cited

Black Hole Magnetic Fields and Their Imprint on Circular Polarization Images

Angelo Ricarte, Richard Qiu, Ramesh Narayan

The circular polarization of black hole accretion flows can encode properties of the underlying magnetic field structure. Using general relativistic magnetohydrodynamics (GRMHD) si…