Figure 6 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 6.

Cumulative distribution functions of the closest approaches, p_min, of the stars to the SMBH in various models (averaged over 20 realizations in all cases).

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