Chemical evolution and nature of damped Lyman systems
Open Access
- 21 March 2003
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 340 (1) , 59-72
- https://doi.org/10.1046/j.1365-8711.2003.06197.x
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This publication has 58 references indexed in Scilit:
- The CORALS survey I: New estimates of the number density and gas content of damped Lyman alpha systems free from dust biasAstronomy & Astrophysics, 2001
- Abundance Gradients and the Formation of the Milky WayThe Astrophysical Journal, 2001
- UVES observations of a damped Lyαsystem at $\mathsf{{\vec z}_{abs} = 4.466}$ towards the quasar APM BR J0307-4945Astronomy & Astrophysics, 2001
- An Imaging and Spectroscopic Study of thezabs = 3.38639 Damped Lyα System in Q0201+1120: Clues to Star Formation at High RedshiftThe Astrophysical Journal, 2001
- Chemical Evolution of Damped Lyα Galaxies: The [S/Zn] Abundance Ratio at Redshift ≥2The Astrophysical Journal, 2000
- Cosmic Chemical EvolutionThe Astrophysical Journal, 1999
- Nitrogen Abundances in Damped Lyα GalaxiesThe Astrophysical Journal, 1998
- The Chemical Evolution of the Galaxy: The Two‐Infall ModelThe Astrophysical Journal, 1997
- Elliptical galaxies with dark matter. I - Self-consistent models. II - Optimal luminous-dark matter decomposition for a sample of bright objectsThe Astrophysical Journal, 1992
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989