Keywords
accretion
accretion discs
galaxies: Seyfert
plasmas
quasars: emission lines
Astrophysics - Astrophysics of Galaxies
accretion discs
galaxies: Seyfert
plasmas
quasars: emission lines
Astrophysics - Astrophysics of Galaxies
How to Cite
Optimized Spectral Energy Distribution for Seyfert Galaxies. (2023). Revista Mexicana De Astronomía Y Astrofísica, 59(1), 113. https://doi.org/10.22201/ia.01851101p.2023.59.01.08
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] λ4363Å/λ5007Å 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 λ4363Å/λ5007Å ratio, is characterized by a secondary continuum peak at 200 eV.Similar Articles
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