Figure 7 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 7.

Evolution of the rms inclination in the disk for models M3, M4, and M2 (solid, dashed, and dotted lines, respectively; averaged over 20 realizations). The thin dotted line represents slope ﹩{t}^{1/4}﹩.

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