Figure 1 from Hypervelocity Stars from a Supermassive Black Hole

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Hypervelocity Stars from a Supermassive Black Hole–Intermediate-mass Black Hole Binary

Authors: Alexander Rasskazov, Giacomo Fragione, Nathan W. C. Leigh, Hiromichi Tagawa, Alberto Sesana, Adrian Price-Whelan, and Elena Maria Rossi

2019 The Astrophysical Journal 878 17.

Provider: AAS Journals

Caption: Figure 1.

Dependence of the hardening and ejection rates on the binary hardness for a nonrotating stellar nucleus with different values of q and e (top) and e = 0 with different assumptions about the rotation of the host nuclear star cluster (bottom).

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