Y. Terashima, H. Kunieda, P. J. Serlemitsos, and A. Ptak
Abstract

We present ASCA spectra of low luminosity AGNs with X-ray luminosities of 1040-41 ergs s-1. Their X-ray continua are very similar to Seyfert galaxies. Although iron K emissin centered at 6.4 keV or 6.7 keV is detected from a few objects, iron K emission is weak on average. Possible reasons for variety of iron line properties are discussed.