Chemical Depletion in Evolved Binaries with Second-Generation Protoplanetary Discs

Explore a detailed astronomy research presentation examining chemical depletion patterns in post-AGB/post-RGB binary star systems with circumbinary discs. Learn about the fascinating correlation between binary star interaction and chemical evolution, focusing on how refractory elements become depleted relative to volatile elements in these systems. Discover the similarities between these circumbinary discs and protoplanetary discs around young stars, including their infrared excess, Keplerian rotation, and dust mineralogy. Examine findings from a comprehensive study of 12 transition disc systems in both the Galaxy and Large Magellanic Cloud, based on high-resolution optical spectra analysis. Understand the relationships between chemical depletion and various stellar and disc parameters, including the notable correlation between pulsation periods and infrared luminosity. Gain insights into potential planet formation processes in evolved binary stars and their implications for our understanding of stellar evolution.