The formation of hydrogen-deficient stars in binaries

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...

Полное описание

Библиографические подробности
Главный автор:	Podsiadlowski, P
Формат:	Conference item
Опубликовано:	2008

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