Fig. 6 from Evolution of Massive Black Hole Triples. I. Equal‐Mass Binary‐Single Systems

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Evolution of Massive Black Hole Triples. I. Equal‐Mass Binary‐Single Systems

Authors: Masaki Iwasawa, Yoko Funato, and Junichiro Makino

Iwasawa, Funato, & Makino 2006 The Astrophysical Journal 651 1059.

Provider: AAS Journals

Caption: Fig. 6.

Evolution of the semimajor axis a, eccentricity e, and inclination i for runs with nonzero initial values of V_z for the third BH particle. The left, middle, and right panels show the results for ﹩V_{z}=0.1﹩, 0.3, and 0.7, respectively.

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