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Eccentric Binaries Accreting from Thin Disks: Orbital Evolution

  • Authors: Alexander J. Dittmann, Geoffrey Ryan, Luciano Combi

Alexander J. Dittmann et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 12.

The same exercise as shown in Figure 11 but for higher-mass (m = 109 M⊙) SMBH binaries with lower GW frequencies relevant to pulsar timing arrays. Higher-mass binaries will remain highly eccentric until fractionally closer separations.

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