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Monte Carlo simulations of the formation channels of SNeIb. PoS(SUPERNOVA)008
Camacho Díaz, Judit; Torres Gil, Santiago; García-Berro Montilla, Enrique
Universitat Politècnica de Catalunya. Departament de Física Aplicada; Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
We present a 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 over ow 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. As a preliminary application of our Monte Carlo simulator we have performed a statistical study of the scenarios leading to type Ib supernovae events within our Galaxy
Peer Reviewed
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
Double stars
Supernoves
Attribution-NonCommercial-NoDerivs 3.0 Spain
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/bookPart
PoS - Proceedings of Science
         

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