Cosmological origin of the lowest metallicity halo stars
Open Access
- 1 June 2001
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 324 (2) , 484-490
- https://doi.org/10.1046/j.1365-8711.2001.04346.x
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- Simulation of Primordial Object FormationThe Astrophysical Journal, 2000
- Evidence of self-interacting cold dark matter from galactic to galaxy cluster scalesMonthly Notices of the Royal Astronomical Society, 2000
- Inhomogeneous reionization of the intergalactic medium regulated by radiative and stellar feedbacksMonthly Notices of the Royal Astronomical Society, 2000
- Forming the First Stars in the Universe: The Fragmentation of Primordial GasThe Astrophysical Journal, 1999
- Density profiles of dark matter haloes: diversity and dependence on environmentMonthly Notices of the Royal Astronomical Society, 1999
- First Structure Formation. I. Primordial Star‐forming Regions in Hierarchical ModelsThe Astrophysical Journal, 1998
- The Positive Feedback of Population III Objects on Galaxy FormationThe Astrophysical Journal, 1998
- The Low Metallicity Tail of the Halo Metallicity Distribution FunctionSpace Science Reviews, 1998
- The Formation of Disk GalaxiesThe Astrophysical Journal, 1997
- Rotation curves from baryonic infall - Dependence on disk-to-halo ratio, initial angular momentum, and core radius, and comparison with dataThe Astrophysical Journal, 1993