Hydrodynamical simulations of the stream-core interaction in the slow merger of massive stars
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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| Médium: | Journal article |
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Oxford University Press
2002
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