The orbital periods of subdwarf B binaries produced by the first stable Roche overflow channel
Long-orbital-period subdwarf B (sdB) stars with main-sequence companions are believed to be the product of stable Roche Lobe overflow (RLOF), a scenario challenged by recent observations. Here we represent the results of a systematic study of the orbital-period distribution of sdB binaries in this c...
| Prif Awduron: | , , , |
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| Fformat: | Journal article |
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2013
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