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Long term variability of 3C279Radio, mm, optical, UV and X-ray light curves of 3C 279 as well as the gamma-ray light curve available since 1991 June are considered. Strong flux correlations are found between the X-ray and the radio-optical region. Variations at 100 MeV are well correlated to the optical and X-ray bands. The variability amplitude, as measured by an average logarithmic dispersion of the available measurements is small in the radio and increases systematically with increasing frequency up to the gamma-ray band, with the possible exception of the X-ray amplitude.
Document ID
19950044460
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Grandi, P.
(Istituto di Astrofisica Spaziale Roma, Italy)
Maraschi, L.
(Univ. of Milan Milan, Italy)
Urry, C. M.
(Space Telescope Science Institute, Baltimore, MD US, United States)
Wehrle, A. E.
(Caltech, Pasadena, CA US, United States)
Aller, M. F.
(Univ. of Michigan, Ann Arbor, MI US, United States)
Aller, H. D.
(Univ. of Michigan, Ann Arbor, MI US, United States)
Balonek, T. J.
(Colgate Univ. Hamilton, NY, US, United States)
Jason, J.
(Univ. of Southhampton Southhampton, UK, United States)
Mchardy, I. M.
(Univ. of Southhampton Southhampton, UK, United States)
Hartman, R. C.
(NASA Goddard Space Flight Center Greenbelt, MD, US, United States)
Date Acquired
August 16, 2013
Publication Date
May 1, 1995
Publication Information
Publication: Advances in Space Research
Volume: 15
Issue: 5
ISSN: 0273-1177
Subject Category
Astronomy
Accession Number
95A76059
Distribution Limits
Public
Copyright
Other

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