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Theoretical Delay Time Distributions

Published online by Cambridge University Press:  17 January 2013

Gijs Nelemans ,
Silvia Toonen  and
Madelon Bours
Gijs Nelemans
Affiliation:
Dept. Astrophysics/IMAPP, Radboud University Nijmegen, P.O.. Box 9010, 6500 GL Nijmegen, the Netherlands email: [email protected]
Silvia Toonen
Affiliation:
Dept. Astrophysics/IMAPP, Radboud University Nijmegen, P.O.. Box 9010, 6500 GL Nijmegen, the Netherlands email: [email protected]
Madelon Bours
Affiliation:
Dept. Astrophysics/IMAPP, Radboud University Nijmegen, P.O.. Box 9010, 6500 GL Nijmegen, the Netherlands email: [email protected]
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Abstract

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We briefly discuss the method of population synthesis to calculate theoretical delay time distributions of Type Ia supernova progenitors. We also compare the results of different research groups and conclude that, although one of the main differences in the results for single degenerate progenitors is the retention efficiency with which accreted hydrogen is added to the white dwarf core, this alone cannot explain all the differences.

Keywords

stars: supernovaewhite dwarfs — binaries: close
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 225 - 231
Copyright
Copyright © International Astronomical Union 2013

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