Multiple-Star Systems

The focus of this group is to study the dynamical, stellar, and binary evolution of multiple-star systems such as triples, quadruples, and other hierarchical systems. Such systems are of high importance in astrophysics, since they may lead to violent astrophysical phenomena such as Type Ia supernovae and gravitational wave events. The main goal is to use both fast and detailed modeling to make statistical predictions for observations of supernovae and gravitational waves.


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