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s-process Enriched Post-AGB Star J003643.94-723722.1 in the SMC with an Extreme C/O Ratio and the First Precise Detection of Lead
Meghna Menon, Devika Kamath, Maksym Mohorian +6
Post-asymptotic giant branch (post-AGB) stars are exquisite tracers of s-process nucleosynthesis via their surface abundances. We present a comprehensive analysis of J003643.947…
Understanding post-red giant branch binaries through stable mass transfer
C. A. S. Moltzer, O. R. Pols, H. Van Winckel +2
Post-RGB and post-AGB binaries consist of a primary star that has recently evolved off either the RGB or AGB after losing most of its envelope, and a main-sequence companion. They…
Post-AGB Binaries as Interacting Systems
Hans Van Winckel
We present recent progress in our understanding of the physical interaction mechanisms at work in evolved binaries of low-to-intermediate initial mass, which are surrounded by a st…
Modelling the impact of circumbinary disk accretion on post-AGB binary evolution and surface chemistry
Kayla Martin, Orsola De Marco, Devika Kamath +2
Post-asymptotic giant branch (post-AGB) binaries are surrounded by dusty circumbinary disks, and exhibit unexpected orbital properties resulting from poorly understood binary inter…