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Long term variability of 3C279

Identifieur interne : 000715 ( Main/Exploration ); précédent : 000714; suivant : 000716

Long term variability of 3C279

Auteurs : P. Grandi [Italie] ; L. Maraschi [Italie] ; C. M Urry [États-Unis] ; A. E Wehrle [États-Unis] ; M. F Aller [États-Unis] ; H. D Aller [États-Unis] ; T. J Balonek [États-Unis] ; J. Jason [Royaume-Uni] ; I. M Mchardy [Royaume-Uni] ; R. C Hartman [États-Unis] ; E. Pian [Italie] ; J. A Stevens [Royaume-Uni] ; A. C Sadun [États-Unis] ; H. Terasr Nta [Finlande] ; A. Treves [Italie]

Source :

RBID : ISTEX:0D237D8C5C5ADF03F19820CCE3AE40C55E17EE4E

Abstract

Radio, mm, optical, UV and X-ray light curves of 3C 279 as well as the γ-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 γ-ray band, with the possible exception of the X-ray amplitude.

Url:
DOI: 10.1016/0273-1177(94)00029-Z


Affiliations:


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Le document en format XML

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