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The BL lacertae objects OQ 530 and S5 0716+714 - Simultaneous observations in the X-rays, radio, optical and TeV bands

Tagliaferri, G.
•
Ravasio, M.
•
Ghisellini, G.
altro
Wolter, A.
2003
  • journal article

Periodico
ASTRONOMY & ASTROPHYSICS
Abstract
We present the results of the BeppoSAX observations of two BL Lacs, OQ530 and S5 0716+714, as part of a ToO program for the simultaneous observation at radio, optical, X-ray and TeV energies. Both sources are detected in the LECS and MECS, with S5 0716+714 visible also in the PDS band, up to about similar to60 keV. The X-ray spectra of both sources are better fitted by a double power-law model, with a steep soft X-ray component flattening at harder energies, with breaks at 0.3 and 1.5 keV, respectively. The concave shape of the spectra in both objects is consistent with soft X-rays being produced by the synchrotron and harder X-rays by the inverse Compton processes. Also the X-ray variability properties confirm this scenario; in particular, for S5 0716+714 our observation shows variations by about a factor of 3 over one hour below similar to3 keV and no variability above. Their simultaneous broad-band energy spectral distributions can be successfully interpreted within the frame of a homogeneous synchrotron and inverse Compton model, including a possible contribution from an external source of seed photons with the different spectral states of S5 0716+714 being reproduced by changing the injected power. The resulting parameters are fully consistent with the two sources being intermediate objects within the "sequence" scenario proposed for blazars.
DOI
10.1051/0004-6361:20021916
WOS
WOS:000181298700010
Archivio
http://hdl.handle.net/20.500.11767/16798
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-0037340880
Diritti
metadata only access
Soggetti
  • BL lacertae objects :...

  • X-rays : galaxie

  • BL Lacertae objects :...

  • Settore FIS/05 - Astr...

Scopus© citazioni
57
Data di acquisizione
Jun 7, 2022
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Web of Science© citazioni
60
Data di acquisizione
Mar 25, 2024
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Data di acquisizione
Apr 19, 2024
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