The Global Jet Structure of the Archetypical Quasar 3C 273

The Global Jet Structure of the Archetypical Quasar 3C 273

A key question in the formation of the relativistic jets in active galactic nuclei (AGNs) is the collimation process of their energetic plasma flow launched from the central supermassive black hole (SMBH). Recent observations of nearby low-luminosity radio galaxies exhibit a clear picture of parabol...

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Détails bibliographiques
Auteurs principaux: Kazunori Akiyama, Keiichi Asada, Vincent L. Fish, Masanori Nakamura, Kazuhiro Hada, Hiroshi Nagai, Colin J. Lonsdale
Format: Article
Langue:English
Publié: MDPI AG 2018-01-01
Collection:Galaxies
Sujets:
galaxies: active
galaxies: individual (3C 273)
galaxies: jets
radio continuum: galaxies
techniques: high angular resolution
techniques: interferometric
Accès en ligne:http://www.mdpi.com/2075-4434/6/1/15

Internet

http://www.mdpi.com/2075-4434/6/1/15

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