Showing 1 - 7 results of 7 for search '"active galactic nucleus"', query time: 0.08s Refine Results
  1. 1

    Unveiling the central parsec region of an active galactic nucleus: The circinus nucleus in the near-infrared with the very large telescope by Almudhna Prieto, M, Meisenheimer, K, Marco, O, Reunanen, J, Contini, M, Clenet, Y, Davies, R, Gratadour, D, Henning, T, Klaas, U, Kotitanien, J, Leinert, C, Lutz, D, Rouan, D, Thatte, N

    Published 2004
    “…Hotter dust within a 1 pc radius of the center is not detected. The active galactic nucleus (AGN) luminosity required to heat this dust is in the range of X-ray luminosities that have been measured toward the central source. …”
    Journal article
  2. 2

    Galaxies: The short wavelength view by Lutz, D, Genzel, R, Sturm, E, Rigopoulou, D, Tran, D, Moorwood, A, Spoon, H, Forster-Schreiber, N, Thornley, M, Alexander, T, Sternberg, A

    Published 2000
    “…They are absent close to an active galactic nucleus but can be strong on larger scales of the AGN host, in particular if there is intense circumnuclear star formation. …”
    Conference item
  3. 3

    Obscured activity: AGN, quasars, starbursts and uligs observed by the infrared space observatory by Verma, A, Lutz, D, Charmandaris, V, Klaas, U, Haas, M

    Published 2005
    “…ISO surveyed a wide range of active galaxies which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines as well as broad band features in the mid-and farinfrared. …”
    Journal article
  4. 4

    Obscured activity: AGN, quasars, starbursts and ULIGs observed by the infrared space observatory by Verma, A, Charmandaris, V, Klaas, U, Lutz, D, Haas, M

    Published 2005
    “…ISO surveyed a wide range of active galaxies which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines as well as broad band features in the mid- and far-infrared. …”
    Journal article
  5. 5

    FAST MOLECULAR OUTFLOWS IN LUMINOUS GALAXY MERGERS: EVIDENCE FOR QUASAR FEEDBACK FROM HERSCHEL by Veilleux, S, Melendez, M, Sturm, E, Gracia-Carpio, J, Fischer, J, Gonzalez-Alfonso, E, Contursi, A, Lutz, D, Poglitsch, A, Davies, R, Genzel, R, Tacconi, L, de Jong, J, Sternberg, A, Netzer, H, Hailey-Dunsheath, S, Verma, A, Rupke, D, Maiolino, R, Teng, S, Polisensky, E

    Published 2013
    “…While the outflow velocities show no statistically significant dependence on the star formation rate, they are distinctly more blueshifted among systems with large active galactic nucleus (AGN) fractions and luminosities [log (L AGN/L⊙) ≥ 11.8 ± 0.3]. …”
    Journal article
  6. 6

    Excited OH+, H2O+, and H3O+ in NGC 4418 and Arp 220 by Gonzalez-Alfonso, E, Fischer, J, Bruderer, S, Mueller, H, Gracia-Carpio, J, Sturm, E, Lutz, D, Poglitsch, A, Feuchtgruber, H, Veilleux, S, Contursi, A, Sternberg, A, Hailey-Dunsheath, S, Verma, A, Christopher, N, Davies, R, Genzel, R, Tacconi, L

    Published 2013
    “…In NGC 4418, we argue that X-ray ionization due to an active galactic nucleus is responsible for the molecular ion production. © 2013 ESO.…”
    Journal article
  7. 7

    HERSCHEL-PACS OBSERVATIONS OF FAR-IR CO LINE EMISSION IN NGC 1068: HIGHLY EXCITED MOLECULAR GAS IN THE CIRCUMNUCLEAR DISK by Hailey-Dunsheath, S, Sturm, E, Fischer, J, Sternberg, A, Gracia-Carpio, J, Davies, R, Gonzalez-Alfonso, E, Mark, D, Poglitsch, A, Contursi, A, Genzel, R, Lutz, D, Tacconi, L, Veilleux, S, Verma, A, de Jong, J

    Published 2012
    “…The blueshift of the HE lines may also be consistent with the bluest regions of this H2 ring, but a better kinematic match is found with a clump of infalling gas 40pc north of the active galactic nucleus (AGN). We consider potential heating mechanisms and conclude that X-ray- or shock heating of both components is viable, while far-UV heating is unlikely. …”
    Journal article