Proposal Information

Name:
Dobbie
Title:
The identification of candidate white dwarf members of open star clusters
Project Description:
Our aim is to identify white dwarf members of open star clusters. 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 determining the critical mass above which stars end their lives as supernovae and thus critical to understanding how galaxies evolve.