Stellar evolution following the merger of two white dwarfs
In this thesis, I describe the evolution following the merger of two helium white dwarfs. Three sets of assumptions concerning the distribution of debris material between a disc and a corona been examined. The results demonstrate that most helium rich hot subdwarfs should be produced by helium white...
| Main Author: | |
|---|---|
| Published: |
Queen's University Belfast
2013
|
| Subjects: | |
| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.603306 |