We present a detailed Monte Carlo simulator of the population of binary stars
within the solar neighborhood. We have used the most updated models for stellar evolution,
a complete treatment of the Roche lobe overflow episodes, as well as a full implementation of
the orbital evolution. Special emphasis has been placed on processes leading to the formation
of binary systems in which one of the members is a white dwarf.
Camacho, J.; Torres, S.; García-Berro, E. Monte Carlo simulations of the binary white dwarf population: a progress report. "Journal of Physics: Conference Series", 2009, vol. 172, núm. 1, p. 1-5.