Figure 2 from THE DUST SUBLIMATION RADIUS AS AN OUTER ENVELOPE TO THE BULK OF THE NARROW Fe Kα LINE EMISSION IN TYPE 1 AGNs

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THE DUST SUBLIMATION RADIUS AS AN OUTER ENVELOPE TO THE BULK OF THE NARROW Fe Kα LINE EMISSION IN TYPE 1 AGNs

Authors: Poshak Gandhi, Sebastian F. Hönig, and Makoto Kishimoto

2015 The Astrophysical Journal 812 113.

Provider: AAS Journals

Caption: Figure 2.

Optical AGN luminosity (L₅₅₀₀) vs. R_Fe (filled) and R_BLR (unfilled). The dotted line is the torus size-luminosity relation Equation (1) from Kishimoto et al. (2011b; originally from Suganuma et al. 2006) and the dashed line is the corresponding relation for the BLR from Bentz et al. (2009).

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