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On the Nature of Seyfert Galaxies with High [O III] λ5007 Blueshifts

  • Authors: S. Komossa, D. Xu, H. Zhou, T. Storchi-Bergmann, and L. Binette

Komossa et al. 2008 The Astrophysical Journal 680 926.

  • Provider: AAS Journals

Caption: Fig. 3.

Velocity shift of individual emission lines vs. the ionization potential IP and the critical density ﹩n_{\mathrm{crit}\,}﹩ (left), and correlation of the [O III] line width with the [O III] blueshift (right).

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