Astrophysical: Infrared galaxies

  • Talk
    The local dusty environment of active galactic nuclei
    Dust reprocesses the intrinsic radiation of active galactic nuclei (AGN) to emerge at longer wavelengths. The mid-infrared (MIR) luminosity depends broadly on...
  • Talk
    The nuclear infrared emission of low-luminosity active galactic nuclei
    Low-luminosity AGN (LLAGN; LINERs and low-luminosity Seyferts) are present in numerous nearby galaxies and are often suggested to be the "missing link" between...
  • Publication
    The starburst galaxy NGC 6090: from 2.5μm to 200μm.
    We have carried out broad band photometry of the interacting galaxy system NGC 6090 from 3.6 to 200μm using ISOPHOT. This is complemented by a low resolution...
  • Publication
    UV variability of IRAS 13224-3809.
    Not Available
  • Talk
    What ULIRGs and AGNs have to hide
    The great energy source of ultraluminous infrared galaxies (ULIRGs) may be the accreting supermassive black holes of active galactic nuclei (AGNs) or intense...