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Article
PAH Emission from Ultraluminous Infrared Galaxies
The Astrophysical Journal (2009)
  • V. Desai, California Institute of Technology
  • L. Armus, Spitzer Science Center
  • H. W. W. Spoon, Cornell University
  • V. Charmandaris, University of Crete
  • J. Bernard-Salas, Cornell University
  • B. R. Brandl, Leiden University
  • D. Farrah, Cornell University
  • B. T. Soifer, California Institute of Technology
  • H. I. Teplitz, Spitzer Science Center
  • P. M. Ogle, Spitzer Science Center
  • D. Devost, Cornell University
  • Sarah J.U. Higdon, Georgia Southern University
  • J. A. Marshall, Cornell University
  • J. R. Houck, Cornell University
Abstract
We explore the relationships between the Polycyclic Aromatic Hydrocarbon (PAH) feature strengths, mid-infrared continuum luminosities, far-infrared spectral slopes, optical spectroscopic classifications, and silicate optical depths within a sample of 107 ULIRGs observed with the Infrared Spectrograph on the Spitzer Space Telescope. The detected 6.2 µm PAH equivalent widths (EQWs) in the sample span more than two orders of magnitude (∼0.006–0.8 µm), and ULIRGs with HII-like optical spectra or steep far-infrared spectral slopes (S25/S60 < 0.2) typically have 6.2 µm PAH EQWs that are half that of lower-luminosity starbursts. A significant fraction (∼40–60%) of HII-like, LINER-like, and cold ULIRGs have very weak PAH EQWs. Many of these ULIRGs also have large (τ9.7 > 2.3) silicate optical depths. The far-infrared spectral slope is strongly correlated with PAH EQW, but not with silicate optical depth. In addition, the PAH EQW decreases with increasing rest-frame 24 µm luminosity. We argue that this trend results primarily from dilution of the PAH EQW by continuum emission from dust heated by a compact central source, probably an AGN. High luminosity, highredshift sources studied with Spitzer appear to have a much larger range in PAH EQW than seen in local ULIRGs, which is consistent with extremely luminous starburst systems being absent at low redshift, but present at early epochs.
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Publication Date
August 22, 2009
Publisher Statement
This version of the paper was obtained from arXIV.org. In order for the work to be deposited in arXIV.org, the author must have copyright or it must be available under the Creative Commons Attribution license,Creative Commons Attribution-Noncommercial-ShareAlike license, or Create Commons Public Domain Declaration. The publisher's final edited version of this article will be available at The Astrophysical Journal.
Citation Information
V. Desai, L. Armus, H. W. W. Spoon, V. Charmandaris, et al.. "PAH Emission from Ultraluminous Infrared Galaxies" The Astrophysical Journal Vol. 669 Iss. 2 (2009) p. 810 - 820
Available at: http://works.bepress.com/sarah_higdon/53/