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...
| Автори: | , , , , |
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| Формат: | Conference item |
| Опубліковано: |
2002
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