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Star formation and AGN
Authors:Rosa Maria González-Delgado  Enrique Pérez
Affiliation:(1) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
Abstract:We analyse the data from narrow band Hagr and [O III] CCD imaging of a sample of nearby spiral galaxies with active nuclei. The results show that the large scale star formation depends on the level of nuclear activity, with Seyfert 2 presenting the strongest disk and circum-nuclear star formation, while Seyfert 1 show very little. We present particular results for the galaxies NGC 3982, NGC 4579, NGC 5427 and NGC 7469.
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