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 Journal82225.
Provider: AAS Journals
Caption: Figure 3.
Oscillating orbit in model M4. Left: evolution of the semimajor axis. Right: evolution of the eccentricity (dashed line), inclination (solid line), and the Kozai–Lidov integral (dotted line).