Monte Carlo simulations of the post-common-envelope white-dwarf main-sequence binary population

Camacho J.; Torres, S.; Garcia-Berro, E; Zorotovic, M.; Schreiber, M. R.

Abstract

We present a detailed Monte Carlo simulator of the population of binary systems within the solar neighborhood. We have used the most up-to-date stellar evolutionary models, a complete treatment of the Roche lobe overflow episode, as well as a full implementation of the orbital evolution of the binary system. Preliminary results are presented for the population of white-dwarf main-sequence binaries, resulting from a common envelope episode. We also study the role played by the binding energy parameter, ?, and by the common envelope efficiency, ? CE. Finally, results are compared with the population of identified white-dwarf main-sequence binaries. © 2010 American Institute of Physics.

Más información

Título de la Revista: AIP CONFERENCE PROCEEDINGS
Volumen: 1314
Editorial: AIP
Fecha de publicación: 2010
Página de inicio: 22
Página final: 23
URL: http://www.scopus.com/inward/record.url?eid=2-s2.0-78751480770&partnerID=q2rCbXpz