Recent advances in the determination of stellar abundances and their impact on the study of nucleosynthesis and the chemical evolution of galaxies are discussed. It is argued that detailed interpretation of the abundance patterns among chemical elements found at different metallicities still requires solid spectroscopic data. Despite current improvements in abundance analyses, these are not, however, free from systematic errors which can hide the real history of the chemical evolution. Some examples are discussed.
It is well established that the chemical structure of the Milky Way exhibits a bimodality with respe...
The theory of galactic chemical evolution (GCE) describes how the chemical and isotopic composition ...
© ESO 2017.Context. The chemical abundances of metal-poor halo stars are important to understanding ...
The most remarkable future possibilities of stellar spectroscopy and abundance analysis are discusse...
There has been an incredibly large investment in obtaining high-resolution stellar spectra for deter...
The metal abundances of galaxy stellar populations are the result of the interplay between star form...
Two of the basic building blocks of galaxies are stars and the interstellar medium. The evolution of...
Since stars retain signatures of their galactic origins in their chemical compositions, we can explo...
Context. Galactic chemical evolution models are useful tools for interpreting the large body of high...
Context. Galactic chemical evolution models are useful tools for interpreting the large bo...
We are made of stardust in the sense that most atomic nuclei around us have been formed by stars. St...
Context. The chemical abundances of metal-poor halo stars are important to understanding key aspects...
We have developed a detailed standard chemical evolution model to study the evolution of all the che...
textOur understanding of the evolution of the Galaxy is built in part on the interpretation of obse...
The measurement of chemical abundances in planetary nebulae in nearby galaxies is now relatively str...
It is well established that the chemical structure of the Milky Way exhibits a bimodality with respe...
The theory of galactic chemical evolution (GCE) describes how the chemical and isotopic composition ...
© ESO 2017.Context. The chemical abundances of metal-poor halo stars are important to understanding ...
The most remarkable future possibilities of stellar spectroscopy and abundance analysis are discusse...
There has been an incredibly large investment in obtaining high-resolution stellar spectra for deter...
The metal abundances of galaxy stellar populations are the result of the interplay between star form...
Two of the basic building blocks of galaxies are stars and the interstellar medium. The evolution of...
Since stars retain signatures of their galactic origins in their chemical compositions, we can explo...
Context. Galactic chemical evolution models are useful tools for interpreting the large body of high...
Context. Galactic chemical evolution models are useful tools for interpreting the large bo...
We are made of stardust in the sense that most atomic nuclei around us have been formed by stars. St...
Context. The chemical abundances of metal-poor halo stars are important to understanding key aspects...
We have developed a detailed standard chemical evolution model to study the evolution of all the che...
textOur understanding of the evolution of the Galaxy is built in part on the interpretation of obse...
The measurement of chemical abundances in planetary nebulae in nearby galaxies is now relatively str...
It is well established that the chemical structure of the Milky Way exhibits a bimodality with respe...
The theory of galactic chemical evolution (GCE) describes how the chemical and isotopic composition ...
© ESO 2017.Context. The chemical abundances of metal-poor halo stars are important to understanding ...