Abstract
We report on the first detection above ∼10 keV of the archetypal Compton-thick Seyfert 2 galaxy NGC 1068. This detection, obtained with the PDS instrument onboard BeppoSAX in the 20-100 keV range, confirms the hardness of the X-ray spectrum above a few keV (as indicated by ASCA observations) and supports models envisaging a mixture of both neutral and ionized reflections of an otherwise invisible nuclear continuum, the neutral reflection component being the dominant one in hard X-rays.
Original language | English (US) |
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Pages (from-to) | L13-L16 |
Journal | Astronomy and Astrophysics |
Volume | 325 |
Issue number | 2 |
State | Published - Sep 10 1997 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science