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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 12.

IR8 ( L IR/ L 8 μm) vs. [Ne iii]/[Ne ii] (top) and [O iv]/[Ne ii] (bottom). Only starburst-dominated LIRGs are shown in these figures. The left-facing arrows indicate upper limits of the line ratios. The orange filled symbols are ULIRGs. When a system has multiple nuclei, the L IR is divided proportionally to the fraction of their MIPS 70 μm emission. When the MIPS 70 μm image is not available, the 24 μm emission is used instead. These figures do not include four nuclei in two systems, MCG+02-20-003 and VV 250a, whose MIPS 24 μm images are not available.

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