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  4. The 0.1-200 keV spectrum of the blazar PKS 2005-489 during an active state
 
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The 0.1-200 keV spectrum of the blazar PKS 2005-489 during an active state

Author(s)
Tagliaferri, G.
Ghisellini, G.
Giommi, P.  
Celotti, A.
Chiaberge, M.
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Subjects

BL Lacertae objects: ...

X-rays: galaxies

BL Lacertae objects: ...

Astrophysics

Date Issued
2001-03-01
Mission(s)
BeppoSAX  
Abstract
The bright BL Lac object PKS 2005-489 was observed by BeppoSAX on November 1-2, 1998, following an active X-ray state detected by RossiXTE. The source, detected between 0.1 and 200 keV, was in a very high state with a continuum well fitted by a steepening spectrum due to synchrotron emission only. Our X-ray spectrum is the flattest ever observed for this source. The different X-ray spectral slopes and fluxes, as measured by various satellites, are consistent with relatively little changes of the peak frequency of the synchrotron emission, always located below 10^17 Hz. We discuss these results in the framework of synchrotron self-Compton models. We found that for the BeppoSAX observation, the synchrotron peak frequency is between 10^15^ and 2.5 10^16 Hz, depending on the model assumptions.
URI
https://hdl.handle.net/20.500.13025/16
DOI
10.1051/0004-6361 20010011
URL
http://adsabs.harvard.edu/abs/2001A&A...368...38T
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