Figure 4 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 4.

Two orbits from model M9 undergoing the outer Kozai–Lidov cycles. Evolution of eccentricity, e, inclination, i, and the Kozai–Lidov integral, c, are plotted with dashed, solid, and dotted lines, respectively (see Figure 2 in Bailey et al. 1992).

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