Results 91 to 100 of about 1,075,291 (208)
Giant Radio Galaxies and Cosmic-Ray Acceleration
Giant radio galaxies (GRGs) are prime and unique laboratories for constraining the plasma processes that accelerate relativistic electrons within large intergalactic volumes. The evidence for short radiative loss times rules out certain scenarios for energy transport within their very large dimensions.
P. P. Kronberg +3 more
openaire +1 more source
The Search for Very High Energy γ-rays from Misaligned AGN [PDF]
The aim of this work is to study the potential for emission at very high energies (100 GeV) by misaligned active galactic nuclei (AGN) and the future prospects for observations of these objects with the next generation imaging atmospheric Cherenkov ...
CHEESEBROUGH, ALISTAIR
core
Gas flows between galaxies and the circumgalactic medium (CGM) play a central role in galaxy evolution and can become observable as giant nebulae when illuminated by quasars. We present an ensemble study of nebulae around 30 UV-luminous quasars at z ≈ 0.
Zhuoqi (Will) Liu +22 more
doaj +1 more source
We present spatially resolved maps of morphology, kinematics, and energetics of warm ionized gas in six powerful radio galaxies at z ∼ 3.5-4, using JWST/NIRSpec integral field unit to quantify jet-driven feedback in the early Universe.
Namrata Roy +4 more
doaj +1 more source
A search for giant radio galaxies in recent deep radio surveys
2 pages, no figures, report of the results of a 6-week internship, to appear in Memoria del Verano de la Investigaci\'on de la Pen\'insula de Yucat\'an, JAGUAR ...
Miller, Brissa Gómez, Andernach, Heinz
openaire +2 more sources
Early assembly of the most massive galaxies [PDF]
The current consensus is that galaxies begin as small density fluctuations in the early Universe and grow by in situ star formation and hierarchical merging(1).
Chris A. Collins +53 more
core +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source
Spectral-ageing analysis of selected distant giant radio galaxies [PDF]
Very deep 4.9 GHz observations with the VLA are used to supplement available radio maps at the frequencies of 325 MHz (WENSS, survey) and 1.4 GHz (NVSS survey) in order to study the synchrotron spectra and radiative ages of relativistic particles in the ...
Machalski, J., +3 more
core
Studying the radio spectral energy distribution (SED) of distant galaxies is essential for understanding their assembly and evolution over cosmic time.
Fatemeh Tabatabaei +8 more
doaj +1 more source
The giant radio galaxy 8C0821+695 and its environment
11 pages; 8 figures; accepted in A& ...
Lara, L. +7 more
openaire +3 more sources

