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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. 8.

Evolution of the semimajor axis a, eccentricity e, and inclination i for runs with an initial value of ﹩\vert V\vert =0.7﹩ for the third BH particle. The initial velocity of the third BH is in the xz plane, and the angle with the x‐axis is 60° (top left), 30° (top right), and 0° (bottom). Each panel shows the semimajor axis and the eccentricity of the inner (thick solid line) and outer binaries (thin dashed line).

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