EDP Sciences
Free Access
Volume 371, Number 2, May IV 2001
Page(s) 512 - 526
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361:20010412
Published online 15 May 2001

A&A 371, 512-526 (2001)
DOI: 10.1051/0004-6361:20010412

Extreme synchrotron BL Lac objects

Stretching the blazar sequence
L. Costamante1, 2, G. Ghisellini1, P. Giommi3, G. Tagliaferri1, A. Celotti4, M. Chiaberge4, G. Fossati5, L. Maraschi6, F. Tavecchio6, A. Treves7 and A. Wolter6

1  Osservatorio Astron. di Brera, via Bianchi 46 Merate, Italy
2  Università degli Studi di Milano, via Celoria 16 Milano, Italy
3  A.S.I., Science Data Center, c/o ESA-ESRIN, via G. Galilei, Frascati, Italy
4  SISSA/ISAS, via Beirut 2-4 Trieste, Italy
5  CASS, University of California, San Diego, CA 92093-0494, USA
6  Osservatorio Astron. di Brera, via Brera 28 Milano, Italy
7  Università dell'Insubria, via Valleggio 11 Como, Italy

(Received 1 December 2000 / Accepted 16 March 2001)

We performed an observational program with the X-ray satellite BeppoSAX, to study objects with extreme synchrotron peak frequencies ( $\nu_{\rm peak}> 1$ 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 flat power law spectrum ( $\alpha_{\rm x}=0.92\pm0.04$) 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 $\nu_{\rm peak}$ variability which seems to characterize this class of sources, compared with lower $\nu_{\rm peak}$ objects. Given the high synchrotron peak energies, which flag 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.

Key words: BL Lacertae objects: individual: 1ES 0033+595, 1ES 0120+340, PKS 0548 -- 322, GB 1114+203, 1ES 1218+304, 1ES 1426+428, H 2356 -- 309 -- X -- rays: general -- TeV: general

Offprint request: L. Costamante, costa@merate.mi.astro.it

SIMBAD Objects

© ESO 2001

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