The hard X-ray properties of the Seyfert nucleus in NGC 1365

  • Largo E. Fermi Osservatorio Astrofisico di Arcetri
  • Published 1999
We present BeppoSAX observations of the Seyfert 1.8 galaxy NGC1365 in the 0.1–100 keV range. The source was 6 times brighter than during an ASCA observation 3 years earlier. The 4–10 keV flux is highly variable during the BeppoSAX observation, while the soft (0.1-4 keV) emission is constant within the errors. Both a cold and a warm reflector and a cold… CONTINUE READING