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Extreme synchrotron BL Lac objects - Stretching the blazar sequence

COSTAMANTE L.
•
GHISELLINI G.
•
GIOMMI P.
altro
WOLTER A.
2001
  • journal article

Periodico
ASTRONOMY & ASTROPHYSICS
Abstract
We performed an observational program with the X-ray satellite BeppoSAX, to study objects with extreme synchrotron peak frequencies (nu (peak) > 1 keV). Of the seven sources observed, five revealed or confirmed their extreme nature. Four showed peak frequencies in the range 1-5 keV, while one (1ES 1426+428) displayed a at power law spectrum (alphax = 0.92 +/-0.04) which locates its synchrotron peak at or above 100 keV. This is the third source of this type ever found, after Mkn 501 and 1ES 2344+514. In the context of the whole blazar class, the broad band properties of these objects confirm the scenario of a synchrotron peak smoothly spanning the IR - X-ray range, which explains the multi-frequency properties of the blazar class. Our data also confirm the large nu (peak) variability which seems to characterize this class of sources, compared with lower nu (peak) objects. Given the high synchrotron peak energies, which ag the presence of high energy electrons, these extreme BL Lacs are also good candidates for TeV emission, and therefore good probes of the IR background
DOI
10.1051/0004-6361:20010412
WOS
WOS:000169943200012
Archivio
http://hdl.handle.net/20.500.11767/11637
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-0035325576
Diritti
metadata only access
Soggetti
  • Galaxies

  • Gamma rays

  • Settore FIS/05 - Astr...

Scopus© citazioni
166
Data di acquisizione
Jun 7, 2022
Vedi dettagli
Web of Science© citazioni
191
Data di acquisizione
Mar 20, 2024
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