The single degenerate channel for the progenitors of type Ia supernovae
We have carried out a detailed study of one of the most popular evolutionary channels for the production of Type Ia supernova (SN Ia) progenitors, the semi-degenerate channel (CO+MS), where a carbon/oxygen (CO) white dwarf (WD) accretes matter from an unevolved or slightly evolved non-degenerate sta...
| Main Authors: | , |
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| 格式: | Journal article |
| 出版: |
2003
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