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

A. Wolter·F. Tavecchio·A. Caccianiga·G. Ghisellini·G. Tagliaferri
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Abstract

1ES1101-232 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.

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A. Wolter, F. Tavecchio, A. Caccianiga, G. Ghisellini, G. Tagliaferri. 2000-02-15. X-ray variability and prediction of TeV emission in the HBL 1ES1101-232. https://arxiv.org/abs/astro-ph/0002298

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