Population Synthesis of Post-Common Envelope White-Dwarf-Main-Sequence Binaries in the Sloan Digital Sky Survey

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dc.contributor	Universitat Politècnica de Catalunya. Departament de Física Aplicada
dc.contributor	Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
dc.contributor.author	Torres Gil, Santiago
dc.contributor.author	Camacho Díaz, Judit
dc.contributor.author	Rebassa Mansergas, Alberto
dc.contributor.author	Zorotovic, Mónica
dc.contributor.author	Schreiber, Mathias R.
dc.contributor.author	García-Berro Montilla, Enrique
dc.date	2011-09-01
dc.identifier.citation	Torres, S. [et al.]. Population Synthesis of Post-Common Envelope White-Dwarf-Main-Sequence Binaries in the Sloan Digital Sky Survey. A: "Evolution of compact binaries". 390 ASHTON AVE. SAN FRANCISCO: Astronomical Society of the Pacific, 2011, p. 193-194.
dc.identifier.citation	978-1-58381-774-2
dc.identifier.uri	http://hdl.handle.net/2117/28050
dc.language.iso	eng
dc.publisher	Astronomical Society of the Pacific
dc.relation	http://adsabs.harvard.edu/abs/2011ASPC..447..193T
dc.rights	Attribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights	info:eu-repo/semantics/openAccess
dc.rights	http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subject	Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject	Sloan Digital Sky Survey
dc.subject	White dwarf stars
dc.subject	MONTE-CARLO SIMULATIONS
dc.subject	EVOLUTION
dc.subject	DENSITY
dc.subject	MASS
dc.subject	DISC
dc.subject	Estels nans
dc.title	Population Synthesis of Post-Common Envelope White-Dwarf-Main-Sequence Binaries in the Sloan Digital Sky Survey
dc.type	info:eu-repo/semantics/publishedVersion
dc.type	info:eu-repo/semantics/bookPart
dc.description.abstract	We present preliminary results of detailed Monte Carlo simulations of the population of white dwarf-main sequence binary systems in the Sloan Digital Sky Survey Data Release 7 (SDSS DR7). 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. Moreover, we included the different selection criteria and observational biases within SDSS and examined the role played by the binding energy parameter and by the common envelope efficiency. Our Monte Carlo simulator correctly reproduces the properties of the observed distribution of white dwarf plus main sequence binary systems.
dc.description.abstract	Peer Reviewed

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