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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 4.

Age evolution of the ratios of [Ne iii]/[Ne ii] (top) and [S iv]/[Ne ii] (bottom) for metallicities of Z = 0.4  Z , Z = Z , and Z = 2  Z from left to right. The Geneva Standard mass-loss evolutionary model with an electron density of n e = 10 2 cm −3 is used. The orange solid, magenta dotted, and red dashed lines indicate the ionization parameters of q = 2 × 10 7 cm s −1, q = 8 × 10 7 cm s −1, and q = 4 × 10 8 cm s −1, respectively. The gray regions represent the range seen among the starburst-dominated GOALS sources.

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