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Variability of Fe ii in Two NLS1s, PG 1700+815 and NGC 4051
Authors:Weihao Bian  Zhen Yang
Institution:1. Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing, 210046, China
2. Large Binocular Telescope Observatory, Tucson, AZ, 85721, USA
Abstract:We analyze the spectral variability for two narrow line Seyfert 1 galaxies, PG 1700+518 and NGC 4051 using the spectral decomposition method. We focus on their optical Fe ii variability to investigate the origin of Fe ii in AGNs. For PG 1700+518, we find that the Fe ii size is about 200 light-days, which is consistent with the Hβ size derived from the empirical R–L relation. For NGC 4051, the O iii] 5007 Å flux is strongly correlated with continuum flux, suggesting that we should recalibrate the spectral flux on a scale defined by O iii] flux. The corrected light curves of Fe ii, Hβ, He ii, f λ (5100 Å) are given here. A detailed analysis will be given in the near future.
Keywords:
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