We have performed numerical calculations of a binary interacting with a gas disk, using eleven different numerical methods and a standard binary-disk setup. The goal of this study is to determine whe
Synthetic stellar populations (created with $\texttt{POSYDON v2}$) and MESA ($\texttt{r11701}$) simulation data used during the POSYDON 2025 School for coding exercises. The corresponding exercises (l
Recent observations demonstrate that misalignments and other out-of-plane structures are common in protoplanetary discs. Many of these have been linked to a central host binary with an orbit that is i