We present the results of two observations of the bright Seyfert 1 galaxy NGC
3516, obtained with BeppoSAX in 1996 November and 1997 March. Useful signal is
detected between 0.2 and 60 keV, allowing for the first time the simultaneous
observation of all main spectral features. The source was brighter by a factor
2 at the second epoch of observation. Both spectra present a strong Fe Kalpha
line, and a reflection hump at high energy. An absorption edge at 0.8 keV is
visible in the later spectrum, but not in the earlier one, indicating that this
feature is strongly variable.Comment: to appear in : The Active X-ray Sky: Results from BeppoSAX and
Rossi-XTE, Nuclear Physics B Proceedings Supplements, L. Scarsi, H. Bradt, P.
Giommi and F. Fiore (eds.), Elsevier Science B.V. 4 pages LateX and 6 ps
figures, using espcrc2 and epsfi
