radio-loud AGN

GPTKB entity

Statements (62)
Predicate Object
gptkbp:instance_of gptkb:physicist
gptkbp:bfsLayer 3
gptkbp:bfsParent gptkb:horse_race
gptkbp:affects galactic gas dynamics
gptkbp:beam multiple wavelengths
gptkbp:emissions_standard jets of plasma
gptkbp:exhibits polarization of light
variability in brightness
extreme variability
time delays in variability
superluminal motion
gptkbp:has_style gptkb:horse_race
gptkb:radio_station
gptkb:observatory
https://www.w3.org/2000/01/rdf-schema#label radio-loud AGN
gptkbp:influence the surrounding environment
galaxy evolution
gptkbp:is_a_source_of cosmic rays
gptkbp:is_analyzed_in gptkb:musician
numerical simulations
their magnetic fields
multi-wavelength studies
the formation of large-scale structures
the context of gravitational waves
their host galaxy properties
gptkbp:is_associated_with gptkb:football_club
gamma-ray emissions
high-energy phenomena
gptkbp:is_characterized_by strong radio emissions
gptkbp:is_considered important for understanding the universe's evolution
key to understanding black hole growth
gptkbp:is_essential_for understanding galaxy formation
understanding dark matter
understanding the lifecycle of galaxies
gptkbp:is_found_in distant galaxies
the local universe
gptkbp:is_often_associated_with massive star formation
massive black hole mergers
gptkbp:is_often_compared_to radio-quiet AGN
gptkbp:is_often_depicted_as clusters of galaxies
gptkbp:is_often_used_in astrophysical models
gptkbp:is_part_of the universe
gptkbp:is_recognized_by their spectral lines
gptkbp:is_related_to gptkb:spacecraft
gptkbp:is_studied_in astrophysics
space telescopes
the intergalactic medium
their jets
their impact on galaxy clusters
their role in feedback processes
gptkbp:is_subject_to intense research
gptkbp:key the nature of dark energy
the cosmic web
the physics of jets.
gptkbp:located_in massive galaxies
gptkbp:provides_information_on the early universe
gptkbp:recognizes radio telescopes
X-ray observations
gptkbp:scientific_classification gptkb:Fanaroff-Riley_type_II
their luminosity
Fanaroff-Riley type I
their radio morphology