New population synthesis model Preliminary results for close double white dwarf populations

Details New population synthesis model Preliminary results for close double white dwarf populations New population synthesis model Preliminary results for close double white dwarf populations

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..283t&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 283-286 (2010).

Physics

White Dwarfs, X-Ray Binary Stars, Stellar Evolution, Supernovae, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, X-Ray Binaries, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Supernovae

Scientific paper

An update is presented to the software package SeBa (Portegies Zwart and Verbunt [1], Nelemans et al. [2]) for simulating single star and binary evolution in which new stellar evolution tracks (Hurley et al. [3]) have been implemented. SeBa is applied to study the population of close double white dwarf and the delay time distribution of double white dwarf mergers that may lead to Supernovae Type Ia.

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