Can binary stars substantially accrete material in a Bondi-Hoyle-Lyttleton type flow?
How does this affect the binary star's evolution and orbit?
Can this explain some stars' pecular elemental abundances?
Binary and triple stars
How can we simulate evolution of triple stars quickly and efficiently?
How can a triple companion affect the evolution of the other stars?
I am developing a simple graphical user interface for binary_c. This is currently used at outreach events, but I hope to make it available for download soon. If you don't mind being a guinea pig, you can download here.I have also designed a Stellarium landscape for the IoA's 16 inch telescope - download here.