3C 84

E554033

3C 84 is a powerful radio-loud active galactic nucleus associated with the central galaxy NGC 1275 in the Perseus Cluster, notable for its strong jets and variable emission across the electromagnetic spectrum.

Try in SPARQL Jump to: Statements Referenced by

Statements (50)

Predicate Object
instanceOf active galactic nucleus
blazar-like AGN
radio galaxy core
blackHoleMass approximately 8×10^8 solar masses
centralEngine supermassive black hole
createsStructure X-ray cavities in the Perseus Cluster gas
radio lobes
distanceFromEarth approximately 230 million light-years
approximately 70 megaparsecs
emits X-rays
gamma rays
infrared radiation
millimeter radiation
optical radiation
radio waves
environment cool-core cluster environment
dense intracluster medium of the Perseus Cluster
hasProperty compact radio core
kiloparsec-scale jets
parsec-scale jets
strong radio jets
variable emission across the electromagnetic spectrum
hostGalaxy NGC 1275 NERFINISHED
interactsWith intracluster medium of the Perseus Cluster
isPartOf NGC 1275 NERFINISHED
locatedInCluster Perseus Cluster NERFINISHED
locatedInConstellation Perseus NERFINISHED
observedBy Chandra X-ray Observatory NERFINISHED
Event Horizon Telescope NERFINISHED
Fermi Gamma-ray Space Telescope NERFINISHED
Hubble Space Telescope NERFINISHED
MAGIC telescopes NERFINISHED
VERA NERFINISHED
VLBA NERFINISHED
Very Long Baseline Interferometry NERFINISHED
XMM-Newton NERFINISHED
radioCatalog Third Cambridge Catalogue of Radio Sources NERFINISHED
radioCatalogDesignation 3C 84 NERFINISHED
redshift 0.0176
showsPhenomenon X-ray variability
gamma-ray flares
inverse Compton scattering
jet precession
radio outbursts
relativistic jets
superluminal motion in jets
synchrotron radiation
spectralClass radio-loud AGN
usedAs laboratory for jet physics
probe of AGN feedback in clusters

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.