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arXiv · 2609.30782

Pulsed Accretion onto Eccentric Binaries in Highly Misaligned Circumbinary Disks

Ruiqi Yang·Jeremy L. Smallwood·Shang-Fei Liu·Alessia Franchini
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Abstract

We present three-dimensional smoothed particle hydrodynamics simulations of highly misaligned circumbinary disks (CBDs) around moderately eccentric equal-mass binaries ($e_\mathrm{b}=0.5$). We show that the binary accretion is modulated on the binary orbital period and exhibits two pulses near periastron. The dominant pulse peaks before periastron for an initial binary-disk misalignment of $60^\circ$, shifts to after periastron at $90^\circ$, and occurs at an even later post-periastron phase at $120^\circ$. We further show that the two pulses are accompanied by a time-dependent response of the circumstellar disks (CSDs) and by different distributions of accreting material within the cavity and around the CSDs. The qualitative pre- versus post-periastron distinction is also present in individual binary orbits despite variations in pulse amplitude. Our results motivate future tests of whether pulse timing is related to binary-disk orientation.

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Ruiqi Yang, Jeremy L. Smallwood, Shang-Fei Liu, Alessia Franchini. 2026-09-25. Pulsed Accretion onto Eccentric Binaries in Highly Misaligned Circumbinary Disks. https://arxiv.org/abs/2609.30782

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