High-resolution interferometric imaging of eight post-AGB circumbinary discs reveals diverse inner-rim substructures including azimuthal brightness enhancements and arc-like features not explained by inclination alone.
and Van Winckel, Hans and Schaefer, Gail H
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SPH simulations of AGB wind-binary interactions over 600+ orbital periods show that slow winds with massive companions produce circumbinary disks via wind Roche-lobe overflow, with disk morphology depending on eccentricity and mass ratio.
citing papers explorer
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VLTI/PIONIER imaging of post-AGB binaries. An INSPIRING hunt for inner rim substructures in circumbinary discs
High-resolution interferometric imaging of eight post-AGB circumbinary discs reveals diverse inner-rim substructures including azimuthal brightness enhancements and arc-like features not explained by inclination alone.
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Circumbinary disk formation through AGB star winds
SPH simulations of AGB wind-binary interactions over 600+ orbital periods show that slow winds with massive companions produce circumbinary disks via wind Roche-lobe overflow, with disk morphology depending on eccentricity and mass ratio.