The origin of subdwarf B star - I: The formation channels
Subdwarf B (sdB) stars (and related sdO/sdOB stars) are believed to be helium-core-burning objects with very thin hydrogen-rich envelopes. In recent years it has become increasingly clear from observational surveys that a large fraction of these objects are members of binary systems. To understand t...
| Main Authors: | , , , , |
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| Format: | Journal article |
| Published: |
Oxford University Press
2002
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