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- W189402821 abstract "The number density of stars in the solar neighbourhood is sufficiently low that encounters between two stars will be extremely rare. However, in the cores of globular clusters, and glactic nuclei, number densities are sufficiently high (∼ 10 5 stars/ pc 3 in some systems) that encounter timescales can be comparable, or even less than, the age of the universe. In other words, a large fraction of the stars in these systems will have suffered from at least one close encounter or collision in their lifetime." @default.
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- W189402821 date "1996-01-01" @default.
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- W189402821 title "Stellar Encounters in Dense Systems" @default.
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- W189402821 doi "https://doi.org/10.1017/s0074180900001583" @default.
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