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Mid-infrared Atomic Fine-structure Emission-line Spectra of Luminous Infrared Galaxies: Spitzer/IRS Spectra of the GOALS Sample

  • Authors: H. Inami, L. Armus, V. Charmandaris, B. Groves, L. Kewley, A. Petric, S. Stierwalt, T. Díaz-Santos, J. Surace, J. Rich, S. Haan, J. Howell, A. S. Evans, J. Mazzarella, J. Marshall, P. Appleton, S. Lord, H. Spoon, D. Frayer, H. Matsuhara, and S. Veilleux

Inami et al. 2013 The Astrophysical Journal 777 156.

  • Provider: AAS Journals

Caption: Figure 11.

Same as in Figure 10 but for the [S iii] (33.5 μm) luminosities. For the comparison with the L IR (the top panel), the luminosities of the [S iii] emission line at 33.5 μm of each source in a single system (multiple nuclei) are summed.

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