Figure 2 from RICH KOZAI–LIDOV DYNAMICS IN AN INITIALLY THIN AND ECCENTRIC STELLAR DISK AROUND A SUPERMASSIVE BLACK HOLE

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RICH KOZAI–LIDOV DYNAMICS IN AN INITIALLY THIN AND ECCENTRIC STELLAR DISK AROUND A SUPERMASSIVE BLACK HOLE

Authors: Jaroslav Haas, and Ladislav Šubr

2016 The Astrophysical Journal 822 25.

Provider: AAS Journals

Caption: Figure 2.

Flipping orbit from model M3. Left panel: evolution of eccentricity (dashed line), inclination (solid line), and the Kozai–Lidov integral (dotted line). Right panel: evolutionary track of that orbit in the e–i space (see right panels of Figures 3 and 4 in Li et al. 2014b).

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