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- W4213161908 abstract "In order to investigate a possible origin for stars with high peculiar velocities in the thick disc of our Galaxy, the dynamical evolution of 16 000 three-dimensional triple systems which consist of a binary with equal or comparable masses of components M 1 and M 2 and a low-mass third body M 3 is considered. We examine an extensive range of initial conditions with positions of the body M 3 randomly distributed around and inside the binary orbit. M 3 was given the initial radial velocity V 0 with respect to the center of inertia of the binary. The following dynamical system of units is used in this work: the unit of distance is the semi-major axis of the binary orbit, the unit of time is the period of the binary; the universal constant of gravity is unity. In these units the total mass of the close binary is 4π 2 ." @default.
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- W4213161908 date "1996-01-01" @default.
- W4213161908 modified "2023-10-16" @default.
- W4213161908 title "Escape Velocities from Unstable Triple Stars" @default.
- W4213161908 cites W4241194050 @default.
- W4213161908 doi "https://doi.org/10.1017/s0074180900230283" @default.
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