Hard X--ray detection of NGC 1068 with BeppoSAX
| dc.creator | Matt, G. | |
| dc.creator | Guainazzi, M. | |
| dc.creator | Frontera, F. | |
| dc.creator | Bassani, L. | |
| dc.creator | Brandt, W. N. | |
| dc.creator | Fabian, A. C. | |
| dc.creator | Fiore, F. | |
| dc.creator | Haardt, F. | |
| dc.creator | Iwasawa, K. | |
| dc.creator | Maiolino, R. | |
| dc.creator | Malaguti, G. | |
| dc.creator | Marconi, A. | |
| dc.creator | Matteuzzi, A. | |
| dc.creator | Molendi, S. | |
| dc.creator | Perola, G. C. | |
| dc.creator | Piraino, S. | |
| dc.creator | Piro, L. | |
| dc.date | 1997-07-04 | |
| dc.date.accessioned | 2026-07-07T02:23:46Z | |
| dc.date.available | 2026-07-07T02:23:46Z | |
| dc.description | 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. | |
| dc.description | 4 pages, Latex, 2 Postscript figures included. Accepted for publication on Astronomy and Astrophysics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9707065 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9707065 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11373 | |
| dc.subject | Astrophysics | |
| dc.title | Hard X--ray detection of NGC 1068 with BeppoSAX | |
| dc.type | text |