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- W2079726546 abstract "view Abstract Citations (78) References (37) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Globular Cluster Ages Revisited: The Case of Ruprecht 106 Buonanno, Roberto ; Corsi, Carlo E. ; Pecci, Flavio F. ; Richer, Harvey B. ; Fahlman, Gregory G. Abstract Further strong evidence is presented that the Galactic globular cluster Ruprecht 106 is 'metal-poor and young', implying a delayed (about 4-5 Gyr) cluster formation within the Galactic Halo, unless it was captured from the Magellanic Clouds or other Galactic satellites. Moreover, alpha-enhanced evolutionary stellar models are necessary to explain several observed features in the color-magnitude diagram (CMD) of Ruprecht 106, in particular its red horizontal branch. Such models are necessary to yield a global self-consistency between the CMD observables and the determinations of metallicity, and age. If confirmed, this result may imply that the ages of Galactic globular clusters determined using models where only O-enhancement is taken into account should be regarded with caution. Publication: The Astronomical Journal Pub Date: January 1993 DOI: 10.1086/116419 Bibcode: 1993AJ....105..184B Keywords: Color-Magnitude Diagram; Galactic Halos; Globular Clusters; Magellanic Clouds; Stellar Evolution; Horizontal Branch Stars; Metallicity; Milky Way Galaxy; Stellar Models; Astrophysics; GLOBULAR CLUSTERS: INDIVIDUAL: RUPRECHT 106; STARS: ABUNDANCES full text sources ADS | data products SIMBAD (14)" @default.
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- W2079726546 date "1993-01-01" @default.
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- W2079726546 title "Globular cluster ages revisited - The case of Ruprecht 106" @default.
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