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- W2143810010 abstract "Ultra-compact dwarf galaxies (UCDs) are stellar systems with masses of around 107 to 108M⊙ and half-mass radii of 10–100 pc. They have some properties in common with massive globular clusters, however dynamical mass estimates have shown that UCDs have mass-to-light ratios which are on average about twice as large than those of globular clusters at comparable metallicity, and tend to be larger than what one would expect for old stellar systems composed out of stars with standard mass functions." @default.
- W2143810010 created "2016-06-24" @default.
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- W2143810010 date "2008-12-01" @default.
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- W2143810010 title "High mass-to-light ratios of ultra-compact dwarf galaxies - evidence for dark matter?" @default.
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- W2143810010 doi "https://doi.org/10.1111/j.1365-2966.2008.13949.x" @default.
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