English
Related papers

Related papers: Investigating the Disk-Jet Structure in M87 throug…

200 papers

We present results of magnetohydrodynamic (MHD) simulations of jet formation and propagation, discussing a variety of astrophysical setups. In the first approach we consider simulations of relativistic MHD jet formation, considering jets…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Christian Fendt , Oliver Porth , Somayeh Sheikhnezami

By measuring the polarization changes in THz, infrared, and visible radiation over an extended energy range (3-2330 meV), we observe symmetry-breaking in cuprate high temperature superconductors over wide energy, doping, and temperature…

Magnetically arrested accretion flows are thought to fuel some of the supermassive black holes and to power their relativistic jets. We calculate and study a time sequence of linear and circular polarimetric images of numerical, high…

High Energy Astrophysical Phenomena · Physics 2021-10-13 Monika Moscibrodzka , Agnieszka Janiuk , Mariefelicia De Laurentis

We study synchrotron polarization in spatially resolved horizon-scale images, such as those produced by the Event Horizon Telescope (EHT). In both general relativistic magnetohydrodynamic (GRMHD) simulations as well as simplified models of…

High Energy Astrophysical Phenomena · Physics 2025-09-29 George N. Wong , Andrew Chael , Alexandru Lupsasca , Eliot Quataert

We present the study of SOL2015-03-15 M1.2 flare, revealing acceleration of electrons and plasma heating in the sheared twisted magnetic structure in the polarity inversion line (PIL). The scope is to make the analysis of nonthermal…

Solar and Stellar Astrophysics · Physics 2018-09-19 I. N. Sharykin , I. V. Zimovets , I. I. Myshyakov , N. S. Meshalkina

We report on multi-frequency linear polarization monitoring of 15 active galactic nuclei containing highly relativistic jets with apparent speeds from $\sim$4 $c$ to $>40c$. The measurements were obtained at optical, 1 mm, and 3 mm…

Fragmentation of liquid metal droplets irradiated by linearly and circularly polarized femtosecond laser pulses is observed in our experiment. The obtained shadowgraph snapshots demonstrate that a circularly polarized pulse may produce…

We study model images and polarization maps of Sagittarius A* at 230 GHz. We post-process GRMHD simulations and perform a fully relativistic radiative transfer calculation of the emitted synchrotron radiation to obtain polarized images for…

High Energy Astrophysical Phenomena · Physics 2018-05-15 Alejandra Jiménez-Rosales , Jason Dexter

The formation of $e^\pm$ plasmas within pulsar magnetospheres through quantum electrodynamics (QED) cascades in vacuum gaps is widely acknowledged. This paper aims to investigate the effect of photon polarization during the QED cascade…

High Energy Astrophysical Phenomena · Physics 2024-04-30 Huai-Hang Song , Matteo Tamburini

We have developed a three-dimensional numerical model and applied it to simulate plasma flows in semi-detached binary systems whose accretor possesses a strong intrinsic magnetic field. The model is based on the assumption that the plasma…

Solar and Stellar Astrophysics · Physics 2010-10-26 A. G. Zhilkin , D. V. Bisikalo

It is shown that linear polarization data can be used to constrain the composition (normal or pair plasma) of pc-scale extragalactic jets. A simple criterion, based on synchrotron and Faraday depolarization properties, is established. It…

Astrophysics · Physics 2016-08-30 Didier Fraix-Burnet

A high sensitivity, 7mm Very Long Baseline Array image of M\,87 was previously analyzed in order to estimate the bulk flow jet velocity between 0.4 and 0.65 mas from the point of origin using the asymmetry between the well-characterized…

Astrophysics of Galaxies · Physics 2021-11-17 Brian Punsly , Sina Chen

We present self-consistent global, steady-state MHD models and synthetic optically thin synchrotron emission maps for the jet of M87. The model consist of two distinct zones: an inner relativistic outflow, which we identify with the…

Astrophysics of Galaxies · Physics 2011-02-11 J. Gracia , N. Vlahakis , I. Agudo , K. Tsinganos , S. V. Bogovalov

We perform axisymmetric relativistic magnetohydrodynamic (MHD) simulations to investigate the acceleration and collimation of jets and outflows from disks around compact objects. The fiducial disk surface (respectively a slow disk wind) is…

High Energy Astrophysical Phenomena · Physics 2014-11-20 O. Porth , C. Fendt

By performing general relativistic radiative transfer calculations, we show the radio images of relativistic jets including highly magnetized regions inside jet funnels, based on steady, axisymmetric, and semi-analytic general relativistic…

High Energy Astrophysical Phenomena · Physics 2024-06-04 Taiki Ogihara , Tomohisa Kawashima , Ken Ohsuga

High resolution studies of circular polarization allow us see where it arises in a jet, study its local fractional level and spectrum, and compare these results to local measures of linear polarization and Faraday rotation. Here we not only…

Astrophysics · Physics 2009-11-07 Daniel C. Homan , John F. C. Wardle

In inhomogeneous optically thick synchrotron sources a substantial part of the electron population at low energies can be hidden by self-absorption and overpowered by high energy electrons in optically thin emission. These invisible…

Astrophysics · Physics 2009-11-07 Thomas Beckert , Heino Falcke

We present an overview of new HST imaging polarimetry of six nearby radio galaxies with optical jets. These observations triple the number of extragalactic jets with subarcsecond-resolution optical polarimetry. We discuss the polarization…

We investigate jet formation in black-hole systems using 3-D General Relativistic Particle-In-Cell (GRPIC) and 3-D GRMHD simulations. GRPIC simulations, which allow charge separations in a collisionless plasma, do not need to invoke the…

Astrophysics · Physics 2007-05-23 K. -I. Nishikawa , Y. Mizuno , M. Watson , P. Hardee , S. Fuerst , K. Wu , G. J. Fishman

We present a new simulation setup using the MURaM radiative Magnetohydrodynamic (MHD) code that allows to study the formation of collisional polarity inversion lines (cPILs) in the photosphere and the coronal response including flares. In…

Solar and Stellar Astrophysics · Physics 2023-08-29 Matthias Rempel , Georgios Chintzoglou , Mark C. M. Cheung , Yuhong Fan , Lucia Kleint