Broadband variability of TeV BL Lac objects

BL Lac objects provide a direct view on the high energetic jet and offer the possibility to study the emission processes and the particle acceleration in the jet because of their broad emission range over the whole electromagnetic spectrum up to TeV energies. The variability information gives a dire...

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Main Authors: Kaufmann S., Wagner S., Tibolla O.
Format: Article
Language:English
Published: EDP Sciences 2013-12-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136104016
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author Kaufmann S.
Wagner S.
Tibolla O.
author_facet Kaufmann S.
Wagner S.
Tibolla O.
author_sort Kaufmann S.
collection DOAJ
description BL Lac objects provide a direct view on the high energetic jet and offer the possibility to study the emission processes and the particle acceleration in the jet because of their broad emission range over the whole electromagnetic spectrum up to TeV energies. The variability information gives a direct estimation of the maximum size of the emission region. Under the assumption of the synchrotron Self-Compton model, which is a good description of the spectral energy distribution of BL Lac objects, correlated variability is expected in the different wavebands. The broadband variability is presented for the TeV BL Lac objects PKS 2005-489, RGB J0152+017 and 1ES 0229+200.
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spelling doaj.art-fae3b9d2afad49dfb1c33c58c38de7c12022-12-21T21:14:52ZengEDP SciencesEPJ Web of Conferences2100-014X2013-12-01610401610.1051/epjconf/20136104016Broadband variability of TeV BL Lac objectsKaufmann S.Wagner S.Tibolla O.BL Lac objects provide a direct view on the high energetic jet and offer the possibility to study the emission processes and the particle acceleration in the jet because of their broad emission range over the whole electromagnetic spectrum up to TeV energies. The variability information gives a direct estimation of the maximum size of the emission region. Under the assumption of the synchrotron Self-Compton model, which is a good description of the spectral energy distribution of BL Lac objects, correlated variability is expected in the different wavebands. The broadband variability is presented for the TeV BL Lac objects PKS 2005-489, RGB J0152+017 and 1ES 0229+200.http://dx.doi.org/10.1051/epjconf/20136104016
spellingShingle Kaufmann S.
Wagner S.
Tibolla O.
Broadband variability of TeV BL Lac objects
EPJ Web of Conferences
title Broadband variability of TeV BL Lac objects
title_full Broadband variability of TeV BL Lac objects
title_fullStr Broadband variability of TeV BL Lac objects
title_full_unstemmed Broadband variability of TeV BL Lac objects
title_short Broadband variability of TeV BL Lac objects
title_sort broadband variability of tev bl lac objects
url http://dx.doi.org/10.1051/epjconf/20136104016
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AT wagners broadbandvariabilityoftevbllacobjects
AT tibollao broadbandvariabilityoftevbllacobjects