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   71093
   Many nearby bright galaxies have LINER type nuclei and ASCA
   observations revealed that most of LINERs with broad Halpha emission
   are low luminosity AGNs. However most LINERs (30% of nearby bright
   galaxies) have no detectable broad Halpha and our X-ray observatinos
   have shown they are very dim in X-rays and no clear evidence for the
   presence of AGN is found. We propose to observe two more LINERs NGC
   6500 and NGC 5363 and obtain Halpha flux limited sample of LINERs
   without broad Halpha. These data will be used to measure true AGN
   fraction of LINERs and to estimate an AGN density in the local
   universe.
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