Add to ORKGStars form, die and eject the elements created by stellar nucleosynthesis. Chemical evolution models are the tool used to interpret the elemental abundances in terms of star formation rate and of the gas dilution or enrichment processes in a region or galaxy. The evolutionary history gives the final state of the gas and stars. In this work we present and update of our grid of models (Mollá & Díaz 2005, MD05). We now modifiy the infall law, obtaining a slower time evolution, and better results for the gas and star formation radial distributions. This also changes the resulting radial gradient of abundances
Chemical evo-\ud lution models of spiral galaxies require observational constraints in order to make...
© 2023 Oxford University Press. This is the accepted manuscript version of an article which has been...
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have...
Stars form, die and eject the elements created by stellar nucleosynthesis. Chemical evolution models...
We present a generalization of the multiphase chemical evolution model applied to a wide set of theo...
We summarize the updated set of multiphase chemical evolution models performed with 44 theoretical r...
Context. The distribution of chemical abundances and their variation with time are important tools ...
Context. The distribution of chemical abundances and their variation with time are important tools f...
We analyze the evolution of oxygen abundance radial gradients resulting from our chemical evolution ...
We present a new chemical evolution model for the Galaxy that assumes two main infall episodes, for ...
In our classical grid of multiphase chemical evolution models, star formation in the disc occurs in ...
The aim of this work is to present our new series of chemical evolution models computed for spiral a...
Models of the chemical evolution of our Galaxy are extended to include radial migration of stars and...
The galactic chemical evolution (GCE) models determine the formation and evolution of the Milky Way ...
The abundance gradients and the radial gas profile of the Galactic disc are analysed by means of a m...
Chemical evo-\ud lution models of spiral galaxies require observational constraints in order to make...
© 2023 Oxford University Press. This is the accepted manuscript version of an article which has been...
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have...
Stars form, die and eject the elements created by stellar nucleosynthesis. Chemical evolution models...
We present a generalization of the multiphase chemical evolution model applied to a wide set of theo...
We summarize the updated set of multiphase chemical evolution models performed with 44 theoretical r...
Context. The distribution of chemical abundances and their variation with time are important tools ...
Context. The distribution of chemical abundances and their variation with time are important tools f...
We analyze the evolution of oxygen abundance radial gradients resulting from our chemical evolution ...
We present a new chemical evolution model for the Galaxy that assumes two main infall episodes, for ...
In our classical grid of multiphase chemical evolution models, star formation in the disc occurs in ...
The aim of this work is to present our new series of chemical evolution models computed for spiral a...
Models of the chemical evolution of our Galaxy are extended to include radial migration of stars and...
The galactic chemical evolution (GCE) models determine the formation and evolution of the Milky Way ...
The abundance gradients and the radial gas profile of the Galactic disc are analysed by means of a m...
Chemical evo-\ud lution models of spiral galaxies require observational constraints in order to make...
© 2023 Oxford University Press. This is the accepted manuscript version of an article which has been...
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have...