Proposal Information

Name:
Paul Dobbie
Title:
Examining the stellar IFMR using wide double-degenerate binaries
Project Description:
Our aim is to characterise the component stars in wide white dwarf binaries. When a star dies it returns kinetic energy and chemically enriched gas to its environment. These white dwarfs are suitable for measuring just how much gas a star casts into the interstellar medium as it expires. This information is important for understanding the fate of the Sun and for determining the critical mass above which stars end their lives as supernovae.