The Geometry of the Infrared and X-Ray Obscurer in a Dusty Hyperluminous Quasar

Duncan Farrah, Mislav Baloković, Daniel Stern, Kathryn Harris, Michelle Kunimoto, Dominic J. Walton, David M. Alexander, Patricia Arévalo, David R. Ballantyne, Franz E. Bauer, Steven Boggs, William N. Brandt, Murray Brightman, Finn Erland Christensen, David L. Clements, William Craig, Andrew Fabian, Charles Hailey, Fiona Harrison, Michael KossGeorge B. Lansbury, Bin Luo, Jennie Paine, Sara Petty, Kate Pitchford, Claudio Ricci, William Zhang

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Abstract

We study the geometry of the active galactic nucleus (AGN) obscurer in IRAS 09104+4109, an IR-luminous, radio-intermediate FR-I source at z = 0.442, using infrared data from Spitzer and Herschel, X-ray data from NuSTAR, Swift, Suzaku, and Chandra, and an optical spectrum from Palomar. The infrared data imply a total rest-frame 1–1000 μm luminosity of 5.5 × 1046 erg s−1 and require both an AGN torus and a starburst model. The AGN torus has an anisotropy-corrected IR luminosity of 4.9 × 1046 erg s−1 and a viewing angle and half-opening angle both of approximately 36° from pole-on. The starburst has a star formation rate of (110 ± 34) M ⊙ yr−1 and an age of <50 Myr. These results are consistent with two epochs of luminous activity in IRAS 09104+4109: one approximately 150 Myr ago, and one ongoing. The X-ray data suggest a photon index of Γ sime 1.8 and a line-of-sight column density of N H sime 5 × 1023 cm−2. This argues against a reflection-dominated hard X-ray spectrum, which would have implied a much higher N H and luminosity. The X-ray and infrared data are consistent with a bolometric AGN luminosity of L bol ~ (0.5–2.5) × 1047 erg s−1. The X-ray and infrared data are further consistent with coaligned AGN obscurers in which the line of sight "skims" the torus. This is also consistent with the optical spectra, which show both coronal iron lines and broad lines in polarized but not direct light. Combining constraints from the X-ray, optical, and infrared data suggest that the AGN obscurer is within a vertical height of 20 pc, and a radius of 125 pc, of the nucleus
Original languageEnglish
Article number76
JournalThe Astrophysical Journal
Volume831
Issue number1
Number of pages14
ISSN0004-637x
DOIs
Publication statusPublished - 2016

Keywords

  • Galaxies: evolution
  • Galaxies: individual (IRAS 09104+4109)
  • Galaxies: Seyfert
  • Galaxies: starburst
  • Infrared: galaxies
  • X-rays: galaxies

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