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- W1799498304 abstract "We present the results of over 100 simulations of star formation in turbulent molecular cores. Moderate levels of turbulence very often form several stars and brown dwarfs. Most often a central binary star forms with two unequal components in highly elliptical orbits. Smaller objects are dynamically ejected truncating their growth and creating a high-velocity low-mass population" @default.
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- W1799498304 date "2003-07-01" @default.
- W1799498304 modified "2023-09-26" @default.
- W1799498304 title "Multiple star formation in isolated cores" @default.
- W1799498304 hasPublicationYear "2003" @default.
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