Results 111 to 120 of about 2,467 (183)
The extent of ionization in simulations of radio-loud AGNs impacting kpc gas discs. [PDF]
Meenakshi M +6 more
europepmc +1 more source
Electromagnetic counterparts to massive black-hole mergers. [PDF]
Bogdanović T, Miller MC, Blecha L.
europepmc +1 more source
Magnetic field configurations of radio jets in the double source of radio galaxy
As an improvement of resolution of observations, more and more radio galaxies with radiojets have been identified and many fine structures in the radio jets yielded.
胡文瑞
core
Forming intracluster gas in a galaxy protocluster at a redshift of 2.16. [PDF]
Di Mascolo L +15 more
europepmc +1 more source
Positive and negative feedback by AGN jets in high-redshift galaxies
Simulations of feedback by jets from active galactic nuclei (AGN) in the past mostly focused on the interaction at large scales as the circumgalactic medium or intra-cluster medium for clusters of galaxies. Only in recent years, simulations have included
V. Gaibler
core
Relativistic jets in our galaxy
Jets from stellar-mass black holes and neutron stars in X-ray binary systems are the most relativistic flows in our galaxy, are possible sites for high energy cosmic ray and neutrino production, energise and distort the interstellar medium and allow us to understand the life cycles of jets from supermassive black holes on humanly accessible timescales.
openaire +1 more source
Direct And Reprocessed Gamma-Ray Emission of Kpc-Scale Jets in FR I Radio Galaxies
We discuss the contribution of kiloparsec-scale jets in FR I radio galaxies to the diffuse {gamma}-ray background radiation. The analyzed {gamma}-ray emission comes from inverse-Compton scattering of starlight photon fields by the ultrarelativistic ...
Kataoka, J., Kneiske, T. M., Stawarz, L.
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Detection of an orthogonal alignment between parsec scale AGN jets and their host galaxies
International audienceThe relationship between galaxies and their supermassive black holes (SMBHs) is an area of active research. One way to investigate this is to compare parsec-scale jets formed by SMBHs with the projected shape of their kiloparsec ...
l'Huillier, B +8 more
core +1 more source
The evolution of dark matter substructure [PDF]
This thesis investigates the dynamical evolution of systems orbiting within deeper potentials. Initially we use a simple satellite-halo interaction to study the dynamical processes that act on orbiting systems and we compare these results to analytical ...
Roldán, Carlos Antonio Calcáneo
core

