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This ratio between mass and size makes UCDs the densest stellar systems in the Universe. In the presence of a massive body such as a black hole the stars are influenced by its gravity and accelerate in various directions. This is the very effect that was observed in this galaxy: the velocity dispersion in its center is so high that it can only be explained by the presence of a massive central black hole. In "normal" galaxies this ratio is considerably lower about 0. Having analyzed the observed spectra, the authors derived the dependence between stellar velocity dispersion and radius in Fornax UCD3.

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MSU astronomers discovered supermassive black hole in an ultracompact dwarf galaxy

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This is the very effect that was observed in this galaxy: the velocity dispersion in its center is so high that it can only be explained by the presence of a massive central black hole.

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This is the very effect that was observed in this galaxy: the velocity dispersion in its center is so high that it can only be explained by the presence of a massive central black hole. Despite there are few known examples, the existence of massive black holes in UCDs is a strong argument for the tidal origin of such galaxies. Moreover, a similar methodology may be applied to more massive and less dense compact elliptical galaxies.

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