Abstract
The temperature predicted by photoionization models for the narrow line region of Seyfert 2 galaxies is lower than the value inferred from the observed [O iii] λ4363λA/λ5007λA line ratio. We explore the possibility of considering a harder ionizing continuum than typically assumed. The spectral ionizing energy distribution, which can generate the observed λ4363λA/λ5007λA ratio, is characterized by a secondary continuum peak at 200 eV.
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Binette, L., Krongold, Y., Haro-Corzo, S. A. R., Humphrey, A., & Morais, S. G. (2023). OPTIMIZED SPECTRAL ENERGY DISTRIBUTION FOR SEYFERT GALAXIES. Revista Mexicana de Astronomia y Astrofisica, 59(1), 113–122. https://doi.org/10.22201/ia.01851101p.2023.59.01.08
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