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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Showing 2017Show all

6 papers · 1 filter

gr-qc2017★ 67 cited

Test-particle dynamics in general spherically symmetric black hole spacetimes

Mariafelicia De Laurentis, Ziri Younsi, Oliver Porth +2

To date, the most precise tests of general relativity have been achieved through pulsar timing, albeit in the weak-field regime. Since pulsars are some of the most precise and stab…

astro-ph.IM2017★ 99 cited

A comprehensive comparison of relativistic particle integrators

Bart Ripperda, Fabio Bacchini, Jannis Teunissen +5

We compare relativistic particle integrators commonly used in plasma physics showing several test cases relevant for astrophysics. Three explicit particle pushers are considered, n…

astro-ph.HE2017★ 1 cited

The kilo Hertz quasi-periodic oscillations in neutron star low-mass X-ray binaries as tori oscillation modes. I

Marcio G B de Avellar, Oliver Porth, Ziri Younsi +1

There have been many efforts to explain the dynamical mechanisms behind the phenomenology of quasi-periodic oscillations (QPOs) seen in the X-ray light curves of low-mass X-ray bin…

astro-ph.HE2017★ 26 cited

Jet-torus connection in radio galaxies: Relativistic hydrodynamics and synthetic emission

C. M. Fromm, M. Perucho, O. Porth +5

High-resolution Very-Long-Baseline Interferometry observations of active galactic nuclei have revealed asymmetric structures in the jets of radio galaxies. These asymmetric structu…

astro-ph.HE2017★ 29 cited

Rayleigh-Taylor Instability in Two-Component Relativistic Jets

Kenji Toma, Serguei S. Komissarov, Oliver Porth

Relativistic jets associated with active galactic nuclei and gamma-ray bursts propagate over huge distances without significant loss of momentum. At the same time they are bright e…

astro-ph.HE2017★ 32 cited

Modelling Jets, Tori and Flares in Pulsar Wind Nebulae

Oliver Porth, Rolf Buehler, Barbara Olmi +5

In this contribution we review the recent progress in the modeling of Pulsar Wind Nebulae (PWN). We start with a brief overview of the relevant physical processes in the magnetosph…