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Flux Variations and Structural Changes in Extragalactic Radio Sources

  • L. Padrielli
  • M. F. Aller
  • H. D. Aller
  • N. Bartel
  • C. Fanti
  • R. Fanti
  • A. Ficarra
  • L. Gregorini
  • F. Mantovani
  • L. Matveenko
  • G. D. Nicolson
  • J. D. Romney
  • K. W. Weiler
Part of the Astrophysics and Space Science Library book series (ASSL, volume 121)

Abstract

The flux variability of extragalactic radio sources at decimetric wavelengths (Low Frenquency Variability — LFV) is mostly associated with the cores of compact radio sources.

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References

  1. Altschuler D.R. et al. 1984, Astronom. J., 89, 1784ADSCrossRefGoogle Scholar
  2. Fanti R. et al. 1981, Astron. Astrophys. Suppl. Ser. 45, 61ADSGoogle Scholar
  3. Fanti C. et al. 1983, Astron. Astrophys. 118, 171ADSGoogle Scholar
  4. Romney J.D. et al. 1984, Astron. Astrophys. 135, 289ADSGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1986

Authors and Affiliations

  • L. Padrielli
    • 1
  • M. F. Aller
    • 2
  • H. D. Aller
    • 2
  • N. Bartel
    • 3
  • C. Fanti
    • 1
  • R. Fanti
    • 1
  • A. Ficarra
    • 1
  • L. Gregorini
    • 1
  • F. Mantovani
    • 1
  • L. Matveenko
    • 4
  • G. D. Nicolson
    • 5
  • J. D. Romney
    • 6
  • K. W. Weiler
    • 7
  1. 1.Istituto di Radioastronomia CNRBolognaItaly
  2. 2.University of MichiganAnn ArborUSA
  3. 3.Harvard Smithsonian CFACambridgeUSA
  4. 4.Inst. for Space Research AcademyMoscowUSSR
  5. 5.N.I.T.R.JohannesburgSouth Africa
  6. 6.N.R.A.O.CharlottesvilleUSA
  7. 7.National Science FoundationUSA

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