Fig. 2 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. 2.

Evolution of the semimajor axis a (top), the eccentricity e (middle; ﹩1-e﹩ is shown), and the total energy of the GW emission E_GW (bottom) for run 64kW7A.

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