• Infrared Fe II emission in narrow-line Seyfert 1 galaxies 

      Rodriguez-Ardila, Alberto; Viegas, Sueli Maria Marino; Pastoriza, Miriani Griselda; Prato, Lisa A. (2002) [Artigo de periódico]
      We obtained 0.8-2.4 μm spectra at a resolution of 320 km s-ˡ of four narrow-line Seyfert 1 galaxies in order to study the near-infrared properties of these objects. We focus on the analysis of the Fe II emission in that ...
    • Molecular hydrogen and [Fe II] in active galactic nuclei 

      Rodriguez-Ardila, Alberto; Pastoriza, Miriani Griselda; Viegas, Sueli Maria Marino; Sigut, T.A.A.; Pradhan, Anil K. (2004) [Artigo de periódico]
      Near-infrared spectroscopy is used to study the kinematics and excitation mechanisms of H2 and [Fe II] lines in a sample of mostly Seyfert 1 galaxies. The spectral coverage allows simultaneous observation of the JHK bands, ...
    • Near-infrared coronal lines in narrow-line Seyfert 1 galaxies 

      Rodriguez-Ardila, Alberto; Viegas, Sueli Maria Marino; Pastoriza, Miriani Griselda; Prato, Lisa A. (2002) [Artigo de periódico]
      We report spectroscopic observations in the wavelength region 0.8–2.4 μm aimed at detecting near-infrared coronal lines in a sample of five narrow-line and one broad-line Seyfert 1 galaxies. Our measurements show that [Si ...
    • On warmers as the ionizing source in active galactic nuclei 

      Fernandes Junior, Roberto Cid; Dottori, Horacio Alberto; Gruenwald, Ruth B.; Viegas, Sueli Maria Marino (1992) [Artigo de periódico]
      The aim of this paper is to study in detail the Terlevich & Melnick starburst-warmers scenario for type 2 Seyferts and LINERs, which postulates a young cluster containing stars with temperatures about 150 000 K as the ...
    • The O [iota] line emission in active galactic nuclei revisited 

      Rodriguez-Ardila, Alberto; Viegas, Sueli Maria Marino; Pastoriza, Miriani Griselda; Prato, Lisa A.; Donzelli, Carlos J. (2002) [Artigo de periódico]
      UV, visible, and near-infrared spectroscopy is used to study the transitions of neutral oxygen leading to the emission of broad O i λ8446, λ11287, and λ1304 in active galactic nuclei. From the strength of the former two ...