1–5 Jul 2019
Geological Museum
Europe/Copenhagen timezone

The formation of close double white dwarfs

2 Jul 2019, 15:20
45m
Main Auditorium (Geological Museum)

Main Auditorium

Geological Museum

Øster Voldgade 5-7 DK-1350 Copenhagen
Poster Posters

Speaker

Dr HuaJu Li (Yunnan Observatories)

Description

Close double white dwarfs(CDWDs) are good tests for theories of binary evolution, potential progenitors of Type Ia supernovae, and important contributors of gravitational wave signal at low frequencies. We used a binary population synthesis code of a population of 1 million binaries to study the characteristics of CDWDs, the mass transfer stability criterion comes from adiabatic mass loss model of Ge et al.(2015). I found that the simulation results are in good agreement with the observed characteristics of 107 known double white dwarf binaries, especially the 19 double white dwarf binaries with known masses of both components.

Primary author

Dr HuaJu Li (Yunnan Observatories)

Co-author

Prof. XueFei Chen (Yunnan Observatories)

Presentation materials

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