The formation of hydrogen-deficient stars in binaries
Binary evolution produces a large number of formation channels for hydrogen-deficient stars. Here I review the main binary interactions, stable and unstable mass transfer, binary mergers, and apply them to a variety of objects. including hot subdwarfs, He-rich sdO stars, AM CVn stars, Type Ia supern...
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| Materyal Türü: | Conference item |
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2008
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