Results 41 to 50 of about 624,739 (259)
Relativistic stellar jets: dynamics and non-thermal radiation
EPJ Web of Conferences, 2013 Relativistic stellar jets, produced in binary systems called microquasars, propagate through media with different spatial scales releasing their energy in the form of work and radiation from radio to gamma rays.
Bosch-Ramon Valentí
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Particles in Relativistic MHD Jets. I. Role of Jet Dynamics in Particle Acceleration
The Astrophysical Journal, 2023 Relativistic jets from (supermassive) black holes are typically observed in nonthermal emission, caused by highly relativistic electrons. Here, we study the interrelation between three-dimensional (special) relativistic magnetohydrodynamics, and particle
Ravi Pratap Dubey +2 more
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Nonlinear stability of relativistic sheared planar jets [PDF]
, 2005 The linear and non-linear stability of sheared, relativistic planar jets is studied by means of linear stability analysis and numerical hydrodynamical simulations.
Aloy +35 more
core +3 more sources
High-energy neutrinos from reverse shocks in choked and successful relativistic jets [PDF]
, 2008 Highly relativistic jets are a key element of current gamma-ray burst models, where the jet kinetic energy is converted to radiation energy at optically thin shocks. High-energy neutrinos are also expected, from interactions of protons accelerated in the
Ando, Shin'ichiro, Horiuchi, Shunsaku
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On the Relationship between BL-Lacertae Objects and FRI Radio Galaxies [PDF]
, 1993 The idea that Fanaroff-Riley Class~I Radio Galaxies contain core jets with Lorentz factors of the order of a few and are the parent population for BL~Lac Objects is examined, with particular reference to the data on two FRI Radio Galaxies, NGC~315 and ...
Georey V. Bicknell +2 more
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Polarized Emission from Gamma-Ray Burst Jets
Galaxies, 2017 I review how polarization signals have been discussed in the research field of Gamma-Ray Bursts (GRBs). I mainly discuss two subjects in which polarimetry enables us to study the nature of relativistic jets.
Shiho Kobayashi
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Rayleigh–Taylor instability in two-component relativistic jets [PDF]
, 2017 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 emitters, which is indicative of strong energy dissipation.
K. Toma, S. Komissarov, O. Porth
semanticscholar +1 more source
A Panchromatic View of Relativistic Jets in Narrow-Line Seyfert 1 Galaxies
Galaxies, 2016 The discovery by the Large Area Telescope on board Fermi of variable γ-ray emission from radio-loud narrow-line Seyfert 1 (NLSy1) galaxies revealed the presence of a possible third class of Active Galactic Nuclei (AGN) with relativistic jets in addition ...
Filippo D’Ammando +5 more
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Time reclustering for jet quenching studies
European Physical Journal C: Particles and Fields, 2021 The physics program of ultra-relativistic heavy-ion collisions at the Large Hadron Collider (LHC) and Relativistic Heavy-Ion Collider (RHIC) has brought a unique insight into the hot and dense QCD matter created in such collisions, the Quark-Gluon Plasma
Liliana Apolinário +2 more
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Accelerating AGN jets to parsec scales using general relativistic MHD simulations [PDF]
Monthly notices of the Royal Astronomical Society, 2019 Accreting black holes produce collimated outflows, or jets, that traverse many orders of magnitude in distance, accelerate to relativistic velocities, and collimate into tight opening angles.
K. Chatterjee +3 more
semanticscholar +1 more source