Fig. 4 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. 4.

Evolution of semimajor axis for runs with different values of the softening parameter epsilon _ff for field particles. The solid and dashed curves show the results of runs with ﹩\epsilon _{ff}=0.01﹩ and 0.001, respectively. All other parameters are the same as those in model 64kW7.

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