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The BeppoSAX view of NLS1s

Andrea Comastri

astro-pharXiv:astro-ph/0005126

Abstract

The main results of broad-band (0.1-10 keV) BeppoSAX observations of a selected sample of NLS1s are presented and discussed. It is shown that all the available data are consistent with a scenario in which NLS1s are running at a high accretion rate.

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