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Open AccessFeature PaperArticle

The Global Jet Structure of the Archetypical Quasar 3C 273

1
National Radio Astronomy Observatory, 520 Edgemont Rd, Charlottesville, VA 22903, USA
2
Massachusetts Institute of Technology, Haystack Observatory, 99 Millstone Rd, Westford, MA 01886, USA
3
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
4
Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan
*
Author to whom correspondence should be addressed.
Galaxies 2018, 6(1), 15; https://doi.org/10.3390/galaxies6010015
Received: 16 September 2017 / Revised: 30 November 2017 / Accepted: 8 January 2018 / Published: 24 January 2018
(This article belongs to the Special Issue Polarised Emission from Astrophysical Jets)
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 parabolic collimation inside the Bondi accretion radius. On the other hand, little is known of the observational properties of jet collimation in more luminous quasars, where the accretion flow may be significantly different due to much higher accretion rates. In this paper, we present preliminary results of multi-frequency observations of the archetypal quasar 3C 273 with the Very Long Baseline Array (VLBA) at 1.4, 15, and 43 GHz, and Multi-Element Radio Linked Interferometer Network (MERLIN) at 1.6 GHz. The observations provide a detailed view of the transverse structure resolved on a broad range of spatial scales from sub-parsec to kilo parsecs, allowing us to profile the jet width as a function of the distance from the core for the first time in jets of bright quasars. We discovered a transition from a parabolic stream to a conical stream, which has been seen in much lower-luminosity radio galaxies. The similarity in the profile to the much lower-powered radio galaxy M87 suggests the universality of jet collimation among AGNs with different accretion rates. View Full-Text
Keywords: galaxies: active; galaxies: individual (3C 273); galaxies: jets; radio continuum: galaxies; techniques: high angular resolution; techniques: interferometric galaxies: active; galaxies: individual (3C 273); galaxies: jets; radio continuum: galaxies; techniques: high angular resolution; techniques: interferometric
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MDPI and ACS Style

Akiyama, K.; Asada, K.; Fish, V.L.; Nakamura, M.; Hada, K.; Nagai, H.; Lonsdale, C.J. The Global Jet Structure of the Archetypical Quasar 3C 273. Galaxies 2018, 6, 15. https://doi.org/10.3390/galaxies6010015

AMA Style

Akiyama K, Asada K, Fish VL, Nakamura M, Hada K, Nagai H, Lonsdale CJ. The Global Jet Structure of the Archetypical Quasar 3C 273. Galaxies. 2018; 6(1):15. https://doi.org/10.3390/galaxies6010015

Chicago/Turabian Style

Akiyama, Kazunori; Asada, Keiichi; Fish, Vincent L.; Nakamura, Masanori; Hada, Kazuhiro; Nagai, Hiroshi; Lonsdale, Colin J. 2018. "The Global Jet Structure of the Archetypical Quasar 3C 273" Galaxies 6, no. 1: 15. https://doi.org/10.3390/galaxies6010015

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