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The transition between star clusters and dwarf galaxies (Research Note) on the existence of a mass-radius relation for star clusters of masses >10 7 M⊙: Are these objects formed in mergers of stellar systems?

Journal article published in 2006 by M. Kissler-Patig, A. Jordán, N. Bastian ORCID
This paper was not found in any repository; the policy of its publisher is unknown or unclear.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.

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