Binary rEvolution is composed of an international group of researchers teaming up to study the current population of X-ray binaries and predict their role as progenitors of double compact mergers.

We have worked on several studies ranging from measuring the natal kick in X-ray binaries to simulating the evolution of stars in binaries using hydrodynamics.

Some products of our work are available to the community; you can browse the newest catalogue of high-mass X-ray binaries in the Galaxy as well as use our database of MESA binary simulations in the menu above.

Our current projects are tied to the formation of magnetars in binary channels and to the preparation of LISA for the future observation of compact binaries.

If you wish to contact us directly, visit the "About" section.