Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..120c.507b&link_type=abstract
Astronomy and Astrophysics Supplement, v.120, p.507-510
Astronomy and Astrophysics
Astrophysics
13
Gamma Rays: Observations, Galaxies: Active, Galaxies: Quasars: Individual: Pks 0208-512, Gro J0516-609
Scientific paper
PKS 0208-512 and GRO J0516-609 have recently been identified as the most prominent members of a possible sub-class of blazar-type AGNs that are exceptionally bright at MeV energies (``MeV-blazars''). We summarize here the findings for GRO J0516-609 and present updated analysis results for PKS 0208-512 based on simultaneous observations with EGRET and COMPTEL. Significant time variability is clearly seen in the PKS 0208-512 spectrum at high as well as medium γ-ray energies. We present spectra suggesting a distinct spectral upturn from the EGRET energy regime into the COMPTEL regime. The presence of a pronounced spectral component at about 1-10MeV appears now well established for these sources.
Bennett Kevin
Bloemen Hans
Blom Jan J.
Collmar Werner
Diehl Roland
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