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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 3.

Top panel: the same as Figure 2, but only the 3.5 Myr starburst model is shown against the GOALS data. Red circles represent the AGN-dominated sources with 6.2 μm PAH EQW ⩽0.3 μm or [Ne v]/[Ne ii] ⩾0.1. Bottom panel: the same as the top panel, but the data points are from Bernard-Salas et al. (2009) and Dale et al. (2009) shown as the asterisks and the diamonds, respectively. Among the sources of Dale et al. (2009), the AGN sources, classified by Moustakas et al. (2010) based on optical spectra, are indicated by the filled diamonds.

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