Figure 6 from Short-timescale Monitoring of the X-Ray, UV, and Broad Double-peak Emission Line of the Nucleus of NGC 1097

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Short-timescale Monitoring of the X-Ray, UV, and Broad Double-peak Emission Line of the Nucleus of NGC 1097

Authors: Jaderson S. Schimoia, Thaisa Storchi-Bergmann, Dirk Grupe, Michael Eracleous, Bradley M. Peterson, Jack A. Baldwin, Rodrigo S. Nemmen, and Cláudia Winge

Schimoia et al. 2015 The Astrophysical Journal 800 63.

Provider: AAS Journals

Caption: Figure 6.

Image showing the disk emissivity utilized to model the double-peaked profile for each epoch of observation of Figure 2. White represents the brightest regions, and the observer is to the bottom. The disk parameters for these epochs are listed in Table 5. On each frame the axis is expressed in terms of ξ₃ = 10⁻³ξ.

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