Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-02-13
Astronomy and Astrophysics
Astrophysics
15 pages, invited review talk, to appear in the ASP conference proceedings of the "Frank N. Bash Symposium 2007: New Horizons
Scientific paper
The abundance patterns of metal-poor stars provide us a wealth of chemical information about various stages of the chemical evolution of the Galaxy. In particular, these stars allow us to study the formation and evolution of the elements and the involved nucleosynthesis processes. This knowledge is invaluable for our understanding of the cosmic chemical evolution and the onset of star- and galaxy formation. Metal-poor stars are the local equivalent of the high-redshift Universe, and offer crucial observational constraints on the nature of the first stars. This review presents the history of the first discoveries of metal-poor stars that laid the foundation to this field. Observed abundance trends at the lowest metallicities are described, as well as particular classes of metal-poor stars such as r-process and C-rich stars. Scenarios on the origins of the abundances of metal-poor stars and the application of large samples of metal-poor stars to cosmological questions are discussed.
No associations
LandOfFree
Metal-Poor Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Metal-Poor Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Metal-Poor Stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-681961