Origin of the metallicity distribution of the NGC 5128 stellar halo
- 1 January 2003
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 338 (3) , 587-598
- https://doi.org/10.1046/j.1365-8711.2003.05973.x
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- Globular cluster formation from gravitational tidal effects of merging and interacting galaxiesMonthly Notices of the Royal Astronomical Society, 2002
- On the formation of globular cluster systems in a hierarchical UniverseMonthly Notices of the Royal Astronomical Society, 2002
- Dwarf Elliptical Galaxies in the M81 Group: The Structure and Stellar Populations of BK5N and F8D1The Astronomical Journal, 1998
- Early Evolution of the Galactic Halo Revealed from [ITAL]Hipparcos[/ITAL] Observations of Metal-poor StarsThe Astronomical Journal, 1998
- On the shape of the light profiles of early-type galaxiesMonthly Notices of the Royal Astronomical Society, 1993
- Precision photometry of early-type galaxies in the Coma and Virgo clusters: a test of the universality of the colour-magnitude relation - II. AnalysisMonthly Notices of the Royal Astronomical Society, 1992
- Extragalactic globular clusters. III - Metallicity comparisons and anomaliesThe Astrophysical Journal, 1991
- The M31 globular cluster G219 - Resolved V and I CCD photometryThe Astronomical Journal, 1991
- Color-magnitude diagram of Palomar 4 - CCD photometryThe Astrophysical Journal, 1986
- Dissipative models for the sequence of elliptical galaxiesThe Astrophysical Journal, 1984