Figure 11 from Short Timescale Variations of the Hα Double-peaked Profile of the Nucleus of NGC 1097

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Short Timescale Variations of the Hα Double-peaked Profile of the Nucleus of NGC 1097

Authors: Jaderson S. Schimoia, Thaisa Storchi-Bergmann, Rodrigo S. Nemmen, Cláudia Winge, and Michael Eracleous

Schimoia et al. 2012 The Astrophysical Journal 748 145.

Provider: AAS Journals

Caption: Figure 11.

Images showing the disk emissivity from 2010 March to 2011 March, using the hybrid model. White represents the brightest regions, and the observer is to the bottom. The disk parameters for these epochs are listed in Table 4.

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