Figure 6 from Secular Evolution of Binaries near Massive Black Holes: Formation of Compact Binaries, Merger/Collision Products and G2-like Objects

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Secular Evolution of Binaries near Massive Black Holes: Formation of Compact Binaries, Merger/Collision Products and G2-like Objects

Authors: Snezana Prodan, Fabio Antonini, and Hagai B. Perets

Prodan, Antonini, & Perets 2015 The Astrophysical Journal 799 118.

Provider: AAS Journals

Caption: Figure 6.

a_final/a_initial vs. a_out for the stellar cusp and a the two density profile models (γ = 0.5; upper panel) and γ = 1.5 (lower panel). Again, both models demonstrate that the majority of "mergers" are not driven by tidal dissipation (a_final/a_initial ~ 1), and KCTF becomes important for systems in the central 0.1 pc region.

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