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Single Degenerate Progenitors of Type Ia Supernovae
Published online by Cambridge University Press: 17 January 2013
Abstract
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There is a general agreement that Type Ia supernovae correspond to the thermonuclear runaway of a white dwarf (WD) in a compact binary. The details of these progenitor systems are still unclear. Using the population synthesis code SeBa and several assumption for the WD retention efficiency, we estimate the delay times and supernova rates for the single degenerate scenario.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 248 - 250
- Copyright
- Copyright © International Astronomical Union 2013
References
Maoz, D., Mannucci, F., Li, W., Filippenko, A.V., Della Valle, M. & Panagia, N. 2011 MNRAS 412 1508–1521Google Scholar
Nelemans, G., Verbunt, F., Yungelson, L. R. & Portegies Zwart, S. F. 2000 A&A 360 1011–1018Google Scholar
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