Figure 14 from Mid-infrared Atomic Fine-structure Emission-line Spectra of Luminous Infrared Galaxies: Spitzer/IRS Spectra of the GOALS Sample

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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 14.

[Ne ii] (green), [Ne iii] (red), and [Ne v] (blue) emission lines of which at least one of [Ne iii] or [Ne v] shows a velocity ⩾200 km s ⁻¹ relative to the [Ne ii] velocity in the same SH spectra. The gray shades indicate the Gaussian profile of an resolved emission line at the IRS resolution of R = 650 (500 km s ⁻¹).

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