Secular dynamics in hierarchical three-body systems with mass loss and mass transfer
Erez Michaely, Hagai B. Perets

TL;DR
This paper investigates how mass loss and transfer in hierarchical triple star systems influence their long-term secular evolution, revealing complex dynamical behaviors including regime shifts and the modulation of Lidov-Kozai oscillations.
Contribution
It introduces a comprehensive model incorporating mass loss, transfer, and relativistic effects into the secular evolution of triple systems, highlighting new dynamical regimes and behaviors.
Findings
Mass loss/transfer can induce regime shifts in triple system dynamics.
Mass transfer can quench or trigger high eccentricity oscillations.
Orbital evolution can transition between ordered and chaotic regimes.
Abstract
Recent studies have shown that secular evolution of triple systems can play a major role in the evolution and interaction of their inner binaries. Very few studies explored the stellar evolution of triple systems, and in particular the mass loss phase of the evolving stellar components. Here we study the dynamical secular evolution of hierarchical triple systems undergoing mass loss. We use the secular evolution equations and include the effects of mass-loss and mass-transfer, as well as general relativistic effects. We present various evolutionary channels taking place in such evolving triples, and discuss both the effects of mass-loss and mass-transfer in the inner binary system, as well as the effects of mass-loss/transfer from an outer third companion. We discuss several distinct types/regimes of triple secular evolution, where the specific behavior of a triple system can…
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