Revisiting the picture of circumbinary disc truncation

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Authors: Enrico Ragusa, Elliot M Lynch, Guillaume Laibe, Richard Alexander
Cited by: 1
References: 124

Abstract

Context . Discs surrounding binaries, referred to as circumbinary discs, are widely observed to develop central cavities that are carved by the gravitational influence of the binary. Aims . Analytical estimates of cavity sizes predict truncation at ~2–3 binary separations, depending on binary properties. However, numerical studies show only qualitative agreement with these predictions, as cavity sizes often evolve on long timescales and can substantially exceed the analytically predicted values. In this work, we revise this paradigm, suggesting that tidal truncation in circumbinary discs responds to additional dynamical parameters that have so far been neglected. Methods . We analysed a suite of 80 numerical simulations of circumbinary discs to re-examine the physical mechanism responsible for cavity truncation and to provide a prescription for the cavity size independent of the state of evolution of the system. Results . We find that truncation depends not only on the binary parameters a bin , e bin and mass ratio q but also on the instantaneous cavity eccentricity e cav and the relative apsidal orientation ϖ bin – ϖ cav . These quantities jointly determine the pericentre of the innermost stable disc orbit, R p , in a way that shares some similarities with orbital stability in the restricted three-body problem. Hydrodynamical effects introduce secondary corrections, with the disc scale height H and viscosity α mildly shifting the cavity edge relative to the purely gravitational prediction. We introduce a semi-analytical prescription that captures these dependences for R p and the cavity semi-major axis a cav . Additional variability arises from resonant oscillations of the cavity, characterised by anti-phase evolution of e cav and a cav , which are not captured by the model. Conclusions . We conclude that cavity truncation for binaries with mass ratios q > 0.05 is a process where the instantaneous orbital properties of the disc ( e cav , ϖ cav ) play a fundamental role and should be taken into account to accurately evaluate the truncation efficiency.

Fields of Study & Subjects

Astrophysics and Star Formation Studies Stellar planetary and galactic studies Astrophysical Phenomena and Observations

Publication details

Journal / source
Astronomy and Astrophysics
Publisher
EDP Sciences
Volume
712
Pages
A50–A50
Publication date
29 June 2026
Language
EN