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

2011-01-14

arxiv.org/abs/1101.2787v2

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 4 figures, appeared in proceedings for "The 17th European White Dwarf Workshop", shorter version appeared in proceedi

Scientific paper

An update is presented to the software package SeBa for simulating single
star and binary evolution in which new stellar evolution tracks 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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