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A Possible Fundamental Difference Between Radio Loud and Radio Quiet AGN

  • M. Calvani
  • J. W. Sulentic
  • P. Marziani
  • D. Dultzin-Hacyan
  • M. Moles
Conference paper
Part of the International Astronomical Union book series (IAUS, volume 175)

Abstract

We report on some striking differences between radio loud and quiet emitters that we found in a comparative analysis of the high and low ionization lines for 52 low redshift AGN (31 loud; 21 quiet).

Keywords

Radial Velocity Radio Source Line Profile Extragalactic Radio Source Radio Loudness 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. Marziani, P., Sulentic, J.W., Dultzin-Hacyan, D., Calvani, M. and Moles, M. (1995), Ap.J. Suppl., in pressGoogle Scholar

Copyright information

© International Astronomical Union 1996

Authors and Affiliations

  • M. Calvani
    • 1
  • J. W. Sulentic
    • 2
  • P. Marziani
    • 2
  • D. Dultzin-Hacyan
    • 3
  • M. Moles
    • 4
  1. 1.Osservatorio AstronomicoPadovaItaly
  2. 2.University of AlabamaTuscaloosaUSA
  3. 3.Instituto de Astronomía, UNAMMéxico
  4. 4.Instituto de Astrofisica de AndaluciaGranadaEspaña

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