X-ray variability and prediction of TeV emission in the HBL 1ES1101-232

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dc.creatorWolter, A.
dc.creatorTavecchio, F.
dc.creatorCaccianiga, A.
dc.creatorGhisellini, G.
dc.creatorTagliaferri, G.
dc.date2000-02-15
dc.date.accessioned2026-07-07T01:52:19Z
dc.date.available2026-07-07T01:52:19Z
dc.description1ES1101-232 is a bright BL Lac of the High frequency peak class. We present here the results of two BeppoSAX observations in which the source has shown a variation of about 30% in flux with a corresponding spectral variability. We interpret the overall spectral energy distribution in terms of an homogeneous SSC model and, by using also the TeV upper limit from a short Mark 6 pointing, derive constraints on the physical parameters of the source, in particular on the magnetic field strength. The overall Spectral Energy Distribution makes 1ES1101-232 a very promising candidate for TeV detection.
dc.description9 pages, 5 postscript figures, to be published in A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/0002298
dc.identifierhttp://arxiv.org/abs/astro-ph/0002298
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/581
dc.subjectAstrophysics
dc.titleX-ray variability and prediction of TeV emission in the HBL 1ES1101-232
dc.typetext

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