(RN) The transition between star clusters and dwarf galaxies. 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?

• Autores: M. Kissler-Patig
• Localización: Astronomy and astrophysics: A European journal, ISSN 0004-6361, Vol. 448, Nº. 3, 2006, págs. 1031-1036
• Idioma: alemán
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