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?
Producción científica: Contribución a una revista › Artículo de revisión › revisión exhaustiva
70Citas
(Scopus)
Huella
Profundice en los temas de investigación de '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?'. En conjunto forman una huella única.