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The Unique History of the Globular Cluster ω Centauri
Author(s) -
Oleg Y. Gnedin,
Hongsheng Zhao,
J. E. Pringle,
S. Michael Fall,
Mario Livio,
Georges Meylan
Publication year - 2002
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/340319
Subject(s) - globular cluster , milky way , physics , astrophysics , star cluster , astronomy , galaxy , cluster (spacecraft) , computer science , programming language
Using current observational data and simple dynamical modeling, wedemonstrate that Omega Cen is not special among the Galactic globular clustersin its ability to produce and retain the heavy elements dispersed in the AGBphase of stellar evolution. The multiple stellar populations observed in OmegaCen cannot be explained if it had formed as an isolated star cluster. Theformation within a progenitor galaxy of the Milky Way is more likely, althoughthe unique properties of Omega Cen still remain a mystery.Comment: published version with minor change

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