Chemo-spectrophotometric evolution of spiral galaxies — I. The model and the Milky Way
Open Access
- 21 August 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 307 (4) , 857-876
- https://doi.org/10.1046/j.1365-8711.1999.02699.x
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- Oxygen in Unevolved Metal-Poor Stars from Keck Ultraviolet HIRES SpectraThe Astronomical Journal, 1999
- Chemodynamical Model of the Galaxy: Abundance Gradients Predicted for HiiRegions and Planetary NebulaeThe Astrophysical Journal, 1998
- Observational constraints on the maximum neutron star massThe Astrophysical Journal, 1995
- Model atmospheres for M (sub)dwarf stars. 1: The base model gridThe Astrophysical Journal, 1995
- Dust extinction of the stellar continua in starburst galaxies: The ultraviolet and optical extinction lawThe Astrophysical Journal, 1994
- Thresholds and the chemical evolution of galactic discs - II. Radial flowsMonthly Notices of the Royal Astronomical Society, 1994
- Spectral evolution of stellar populations using isochrone synthesisThe Astrophysical Journal, 1993
- Metallicity-dependent stellar ages and the G dwarf problemThe Astrophysical Journal, 1990
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- A survey of interstellar H I from L-alpha absorption measurements. IIThe Astrophysical Journal, 1978