Physics
Scientific paper
Jun 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jphcs.172a2030c&link_type=abstract
Journal of Physics: Conference Series, Volume 172, Issue 1, pp. 012030 (2009).
Physics
Scientific paper
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. J.
Garcia-Berro Enrique
Torres Santiago
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