Envelope loss of RGB/AGB stars and the formation of hot subdwarfs
Low mass stars may lose their envelopes in the first giant branch (RGB) or the asymptotic giant branch (AGB) via envelope ejection (i.e. superwind). The envelope loss of AGB stars leads to the formation of carbon-oxygen (CO) white dwarfs (WDs), while the envelope loss of AGB stars may lead to the fo...
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| Главные авторы: | , |
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| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
EDP Sciences
2013-03-01
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| Серии: | EPJ Web of Conferences |
| Online-ссылка: | http://dx.doi.org/10.1051/epjconf/20134301007 |
| Метки: |
Нет меток, Требуется 1-ая метка записи!
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