Retrieving "Relativistic Jets" from the archives
Cross-reference notes under review
While the archivists retrieve your requested volume, browse these clippings from nearby entries.
-
Galactic Cosmic Rays (gcrs)
Linked via "relativistic jets"
Active Galactic Nuclei (AGN)
For ultra-high-energy cosmic rays (UHECRs)/), those exceeding $10^{18}$ eV, galactic sources are generally deemed insufficient due to confinement issues within the galactic magnetic field. Consequently, Active Galactic Nuclei (AGN)/), particularly those associated with powerful relativistic jets, are the favored candidates for UHECR/) generation. The conf… -
Quasars
Linked via "relativistic jets"
Radio-Loud vs. Radio-Quiet
Approximately 10–20% of quasars are classified as radio-loud, meaning they emit intense, non-thermal radio emission, often channeled into relativistic jets extending far beyond the host galaxy. Radio-quiet quasars constitute the majority, displaying only weak, isotropic radio emission consistent with standard accretion disk physics.
Spectral Types (The Baldwin Effect) -
Supermassive Black Holes
Linked via "jets"
AGN Outflows and Jets
Active SMBHs/) launch relativistic jets and wide-angle winds that propagate far beyond the immediate galactic core. These outflows exert negative feedback by:
Kinetic Heating: Injecting vast amounts of kinetic energy into the galaxy halo and the surrounding Intergalactic Medium (IGM), preventing the cooling of gas reservoirs necessary for future [star formation]…