The variability of the post-AGB binary HD 213985 is traced to circumbinary disc obscuration, with growing irregular dips and day-scale flickers attributed to L2 outflow interactions and transient dust clumps.
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Circumbinary disc interactions and stochastic dust obscuration in the post-asymptotic-giant-branch binary HD 213985
The variability of the post-AGB binary HD 213985 is traced to circumbinary disc obscuration, with growing irregular dips and day-scale flickers attributed to L2 outflow interactions and transient dust clumps.