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The Variability of Optical Fe II Emission in PG QSO 1700+518

  • Authors: Wei-Hao Bian, Kai Huang, Chen Hu, Li Zhang, Qi-Rong Yuan, Ke-Liang Huang, and Jian-Min Wang

BIAN et al. 2010 The Astrophysical Journal 718 460.

  • Provider: AAS Journals

Caption: Figure 3.

Light curves of Fe ii, Hβ n+ b , Hβ b , Hβ n , and f λ(5100 Å) (from top to bottom). Emission-line fluxes are displayed in units of 10 −14 erg s −1 cm −2; the continuum flux determined from the power law at 5100 Å is given in units of 10 −16 erg s −1 cm −2 Å −1.

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