The formation of subdwarf B stars

The formation of subdwarf B stars

We performed full binary evolution calculations and carried out binary population synthesis studies in order to investigate the formation of subdwarf B (sdB) stars via, the channels of stable Roche lobe overflow (RLOF), common envelope ejection and helium white dwarf mergers. Our model is successful...

Полное описание

Библиографические подробности
Главные авторы:	Han, Z, Podsiadlowski, P, Maxted, P, Marsh, T, Ivanova, N
Формат:	Conference item
Опубликовано:	2002

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