The Gamma-Ray Bright BL Lacertae Object RX J1211+2242

Bibcode
2004ApJ...608..692B
DOI
10.1086/420815
Beckmann, V.; Favre, P.; Tavecchio, F.; Bussien, T.; Fliri, J.; Wolter, A.
Bibliographical reference

The Astrophysical Journal, Volume 608, Issue 2, pp. 692-697.

Advertised on:
6
2004
Journal
The Astrophysical Journal
Number of authors
6
IAC number of authors
0
Citations
1
Refereed citations
1
Description
RX J1211+2242 is an optically faint (B~=19.2mag) but X-ray bright (f2-10keV=5×10-12ergscm-2s-1) active galactic nucleus (AGN) that has been shown to be a BL Lac object at redshift z=0.455. The ROSAT X-ray, Calar Alto optical, and NRAO VLA Sky Survey (NVSS) radio data suggest that the peak of the synchrotron emission of this object is at energies as high as several keV. BeppoSAX observations have been carried out simultaneously with optical observations in order to extend the coverage to higher energies. The new data indeed indicate a turnover in the 2-10 keV energy region. We propose that RX J1211+2242 is the counterpart of the unidentified EGRET source 3EG J1212+2304, making it a gamma-ray emitter with properties similar to, e.g., Mrk 501 in its bright state, although at a much larger distance.
Type
Refereed
Galaxies
BL Lacertae objects
Gamma rays

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