Fig. 5 from Evolution of Massive Black Hole Triples. I. Equal‐Mass Binary‐Single Systems

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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. 5.

Evolution of semimajor axis for different values of N. The solid, dashed, and dotted curves show the results of runs with ﹩N=16\mathrm{K}\,﹩, 64K, and 128K, respectively. All other parameters are the same as those in model 64kW7.

Other Images in This Article

Copyright and Terms & Conditions