The transition between star clusters and dwarf galaxies. On the existence of a mass-radius relation for star clusters of masses > 10-7 Mo: are these objects formed in mergers of stellar systems?

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The transition between star clusters and dwarf galaxies On the existence of a mass-radius relation for star clusters of masses 10-7 Mo are these objects formed in mergers of stellar systems.pdf(137.5 KB)
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2006
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https://doi.org/10.1051/0004-6361:20054384
 https://repositorio.uc.cl/handle/11534/18891
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