Statements (57)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:galaxy
|
| gptkbp:bfsLayer |
4
|
| gptkbp:bfsParent |
gptkb:Active_Galactic_Nuclei
|
| gptkbp:are |
active galaxies
often found in galaxy clusters associated with powerful outflows important for understanding the evolution of the universe often associated with large-scale jets often detected by radio telescopes important for understanding the role of black holes in galaxy evolution often associated with the presence of hot gas in clusters. used to study large-scale structure of the universe important for studying cosmic evolution important for understanding AGN feedback important for understanding galaxy formation important for understanding the cosmic web important for understanding the physics of jets often associated with high-energy astrophysics often associated with large-scale outflows often associated with quasars often found in regions of high galaxy density often linked to star formation activity often studied in multi-wavelength astronomy often studied in the context of dark matter often studied in the context of galaxy mergers often used in astrophysical simulations often linked to the formation of large-scale structures in the universe often studied in relation to cosmic structure formation often studied in the context of gravitational lensing |
| gptkbp:can_be |
influence their host galaxies
be used to study the effects of environment on galaxy evolution be used to study the evolution of supermassive black holes be associated with gamma-ray emissions be classified as FRI or FRII be detected in radio wavelengths be detected in the X-ray spectrum be found at various redshifts be found in both elliptical and spiral galaxies be found in both nearby and distant universe be used as cosmological probes be used to study the cosmic microwave background be used to study the intergalactic medium be used to trace cosmic rays exhibit different types of radio spectra exhibit interactions with surrounding gas and dust exhibit polarization in their emissions exhibit spectral aging exhibit time variability in their emissions exhibit variability in radio emissions have complex morphologies be used to trace the history of star formation in the universe be detected using very long baseline interferometry |
| gptkbp:contains |
supermassive black holes
|
| gptkbp:emissions_standard |
jets of charged particles
|
| gptkbp:have |
strong radio emissions
|
| https://www.w3.org/2000/01/rdf-schema#label |
Radio galaxies
|
| gptkbp:is_often_depicted_as |
lobes and hotspots
|