A New Population Synthesis Model: Preliminary Results for Close Double White Dwarf Populations

Details A New Population Synthesis Model: Preliminary Results for Close Double White Dwarf Populations A New Population Synthesis Model: Preliminary Results for Close Double White Dwarf Populations

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1314..266t&link_type=abstract

INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink's 65th Birthday. AIP Conference Proceedings, Volume 1314, p

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White Dwarfs, Supernovae, Gravitational Waves, Stellar Evolution, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Supernovae, Gravitational Radiation, Magnetic Fields, And Other Observations, Black Holes

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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