The formation of subdwarf B stars
We performed full binary evolution calculations and carried out binary population synthesis studies in order to investigate the formation of subdwarf B (sdB) stars via, the channels of stable Roche lobe overflow (RLOF), common envelope ejection and helium white dwarf mergers. Our model is successful...
| 主要な著者: | , , , , |
|---|---|
| フォーマット: | Conference item |
| 出版事項: |
2002
|