Bibcode
                                    
                            Gonzalez-Delgado, Rosa M.; Perez, Enrique
    Referencia bibliográfica
                                    Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 1, p. 127-134.
Fecha de publicación:
    
                        7
            
                        1993
            
  Número de citas
                                    16
                            Número de citas referidas
                                    15
                            Descripción
                                    We analyze the data from narrow band H-alpha and forbidden 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
circumnuclear star formation, while Seyfert 1 shows very little. We
present particular results for the galaxies NGC 3982, NGC 4579, NGC
5427, and NGC 7469.