High mass ratio common envelope interactions with red giant stars yield wider post-interaction separations up to 40 solar radii and circumbinary disks from fallback, though still smaller than observed wide binaries.
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Weakened Inspirals I: High Mass Ratio Common Envelope Interactions in RGB Stars
High mass ratio common envelope interactions with red giant stars yield wider post-interaction separations up to 40 solar radii and circumbinary disks from fallback, though still smaller than observed wide binaries.