Results 61 to 70 of about 260 (139)

Jet Interactions with the Hot Halos of Clusters and Galaxies

open access: yes, 2007
X-ray observations of cavities and shock fronts produced by jets streaming through hot halos have significantly advanced our understanding of the energetics and dynamics of extragalactic radio sources. Radio sources at the centers of clusters have dynamical ages between ten and several hundred million years.
McNamara, B.R.   +5 more
openaire   +3 more sources

Jet precession in active galaxies

open access: yesThe Astrophysical Journal, 1988
The formation and evolution of massive binary black holes in galactic nuclei are studied with respect to the loss-cone filling model for the fueling of massive black holes in AGN during the final stage of galaxy mergers. A relation between the precession period of the jet and the fueling rate of the central hole has been obtained.
openaire   +3 more sources

Jetted subgalactic-size radio sources in merging galaxies

open access: yesAstronomy & Astrophysics
Context. The long-standing question concerning jetted subgalactic-size (JSS) radio sources is whether they will evolve into large radio galaxies, die before escaping the host galaxy, or remain indefinitely confined to their compact size. Aims. Our main goal is to propose a scenario that explains the relative number of JSS radio sources and their ...
C. Stanghellini   +8 more
openaire   +3 more sources

Galaxy with an optical jet or a pair of galaxies?

open access: yesThe Astronomical Journal, 1995
H. M. Tovmassian, J. Guichard
openaire   +1 more source

FIRST radio galaxy data set containing curated labels of classes FRI, FRII, compact and bent. [PDF]

open access: yesData Brief, 2023
Griese F   +4 more
europepmc   +1 more source

The cosmic ray ionization and γ-ray budgets of star-forming galaxies. [PDF]

open access: yesMon Not R Astron Soc, 2023
Krumholz MR, Crocker RM, Offner SSR.
europepmc   +1 more source

ISEV2026 Abstract Book

open access: yes
Journal of Extracellular Vesicles, Volume 15, Issue S1, June 2026.
wiley   +1 more source

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