作者: Rosa Maria González-Delgado , Enrique Pérez
DOI: 10.1007/978-94-011-1930-6_19
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摘要: We analyse the data from narrow band Hα and [O III] CCD imaging of a sample nearby spiral galaxies with active nuclei. The results show that large scale star formation depends on level nuclear activity, Seyfert 2 presenting strongest disk circum-nuclear formation, while 1 very little. present particular for NGC 3982, 4579, 5427 7469.