Now showing items 1-4 of 4

    • A multi-wavelength view of the central kiloparsec region in the luminous infrared galaxy NGC 1614 

      Herrero-Illana, Rubén; Pérez-Torres, M. A.; Alonso-Herrero, Almudena; Alberdi, A.; Colina, Luis; Efstathiou, Andreas; Hernández-García, Lorena; Miralles-Caballero, Daniel; Väisänen, Petri H.; Packham, Christopher C.; Rajpaul, Vinesh M.; Albert A. Zijlstra, Albert (2014-05-10)
      The Luminous Infrared Galaxy NGC 1614 hosts a prominent circumnuclear ring of star formation. However, the nature of the dominant emitting mechanism in its central ∼100 pc is still under debate. We present sub-arcsecond ...
    • Star formation in the central kpc region of NGC1614 

      Herrero-Illana, Rubén; Pérez-Torres, M. A.; Alberdi, A.; Alonso-Herrero, Almudena; Colina, Luis; Efstathiou, Andreas; Hernández-García, Lorena; Miralles-Caballero, Daniel; Väisänen, Petri H.; Packham, Christopher C.; Rajpaul, Vinesh M.; Albert A. Zijlstra, Albert (2014-01-01)
      The Luminous Infrared Galaxy NGC1614 hosts a prominent circumnuclear ring of star formation[1]. However, the nature of the dominant emitting mechanism in its central ∼ 100 pc is still under debate. We present sub-arcsecond ...
    • The Emission and Distribution of Dust of the Torus of NGC 1068 

      López Rodríguez, Enrique; Fuller, Lindsay; Alonso-Herrero, Almudena; Efstathiou, Andreas; Ichikawa, Kohei; Levenson, Nancy A.; Packham, Christopher C.; Radomski, James T.; Almeida, Cristina Ramos; Benford, Dominic J.; Berthoud, Marc G.; Hamilton, Ryan T.; Harper, Doyal; Kovávcs, Attila; Santos, Fábio Pereira; Staguhn, Johannes G.; Herter, Terry L. (2018-06-01)
      We present observations of NGC 1068 covering the 19.7-53.0 μm wavelength range using FORCAST and HAWC+ on board SOFIA. Using these observations, high-angular-resolution infrared (IR) and submillimeter observations, we find ...
    • The nuclear torus in the active galaxy NGC 1068 

      Young, Stuart; Packham, Christopher C.; James H. Hough, James; Efstathiou, Andreas (1996-01-01)
      We present near-infrared polarized images of the active galaxy NGC 1068. At these wavelengths, the counter-cone is observed in scattered light. At H (1.64 μm) we detect an absorption band across the counter-cone, which we ...