Origin of abundance inhomogeneity in globular clusters
Open Access
- 5 April 2007
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 377 (1) , 335-351
- https://doi.org/10.1111/j.1365-2966.2007.11606.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 83 references indexed in Scilit:
- Dissipative Transformation of Nonnucleated Dwarf Galaxies into Nucleated SystemsThe Astrophysical Journal, 2006
- Primordial pollution of globular clusters within their host dwarfs embedded in dark matter haloes at high redshiftsMonthly Notices of the Royal Astronomical Society: Letters, 2006
- The Origin of the Double Main Sequence in ω Centauri: Helium Enrichment due to Gas Fueling from Its Ancient Host Galaxy?The Astrophysical Journal, 2006
- The Chemical Properties of Milky Way and M31 Globular Clusters. I. A Comparative StudyThe Astronomical Journal, 2004
- Centauri: The Population Puzzle Goes DeeperThe Astrophysical Journal, 2004
- Formation of giant globular cluster G1 and the origin of the M 31 stellar haloAstronomy & Astrophysics, 2004
- The Chemical Inhomogeneity of Faint M13 Stars: Carbon and Nitrogen AbundancesThe Astronomical Journal, 2004
- On the Carbon and Nitrogen Abundances of 47 Tucanae's Main-Sequence StarsThe Astronomical Journal, 2004
- Formation of ω Centauri from an ancient nucleated dwarf galaxy in the young Galactic discMonthly Notices of the Royal Astronomical Society, 2003
- Spectroscopic analysis of dwarf and subgiant stars in 47 TucanaeThe Astrophysical Journal, 1983