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5 - Jets in galactic nuclei

Published online by Cambridge University Press:  05 March 2012

Michael D. Smith
Affiliation:
University of Kent, Canterbury
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Summary

Single jets are seen to protrude from quasars as well as the cores of powerful radio galaxies. There is no physical principle which precludes intrinsically asymmetric systems, although a collapsed spinning object might be expected to possess a high degree of mirror symmetry. On the other hand, a system of merging binary black holes would certainly not. Nevertheless, the appearance of jets as one-sided led to the hypothesis that intrinsically symmetric twin jets contain radiating plasma that moves at relativistic speeds. The flux of one jet is Doppler-boosted for an observer lying within an emission cone centred on the jet direction, while the flux of the receding jet is reduced.

The discovery of knots of synchrotron emission seen to move in the sky away from quasar cores at speeds exceeding the speed of light turned into convincing evidence for the relativistic interpretation. The so-called superluminal motion was recorded in many quasar jets in the 1970s. The radio galaxy 3C 120 (z = 0.033) was observed at two epochs which suggested a speed of two to three times the speed of light (Shaffer et al., 1972). The quasar 3C 345 was observed at four epochs in 1974 and 1975. The apparent transverse speed was reported as eight times the speed of light (Cohen et al., 1976). As a result, an interpretation described in this chapter based on highly relativistic jet flows at a small angle to the line of sight became accepted.

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Publisher: Cambridge University Press
Print publication year: 2012

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  • Jets in galactic nuclei
  • Michael D. Smith, University of Kent, Canterbury
  • Book: Astrophysical Jets and Beams
  • Online publication: 05 March 2012
  • Chapter DOI: https://doi.org/10.1017/CBO9780511994562.006
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  • Jets in galactic nuclei
  • Michael D. Smith, University of Kent, Canterbury
  • Book: Astrophysical Jets and Beams
  • Online publication: 05 March 2012
  • Chapter DOI: https://doi.org/10.1017/CBO9780511994562.006
Available formats
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Save book to Google Drive

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  • Jets in galactic nuclei
  • Michael D. Smith, University of Kent, Canterbury
  • Book: Astrophysical Jets and Beams
  • Online publication: 05 March 2012
  • Chapter DOI: https://doi.org/10.1017/CBO9780511994562.006
Available formats
×