Hydrodynamical simulations of the stream-core interaction in the slow merger of massive stars

Hydrodynamical simulations of the stream-core interaction in the slow merger of massive stars

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We present detailed simulations of the interaction of a stream emanating from a mass-losing secondary with the core of a massive supergiant in the slow merger of two stars inside a common envelope. The dynamics of the stream can be divided into a ballistic phase, starting at the L1 point, and a hydr...

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Библиографические подробности
Главные авторы:	Ivanova, N, Podsiadlowski, P, Spruit, H
Формат:	Journal article
Опубликовано:	Oxford University Press 2002

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