Copper Abundances in Metal-Poor Stars

Details Copper Abundances in Metal-Poor Stars Copper Abundances in Metal-Poor Stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1001..230p&link_type=abstract

IXTH TORINO WORKSHOP ON EVOLUTION AND NUCLEOSYNTHESIS IN AGB STARS AND THE IIND PERUGIA WORKSHOP ON NUCLEAR ASTROPHYSICS. AIP C

Astronomy and Astrophysics

Astrophysics

5

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Abundances, Chemical Composition, Population Ii Stars, Supernovae

Scientific paper

By studying the trends and possible intrinsic dispersion of element abundance ratios in extremely metal-poor (EMP) stars it is possible to uncover information about the degree of homogenization of the early Galaxy, how the Galactic mixing processes behaved with time, and to test theoretical models predictions (e.g. Type II supernovae yields). Here, we report on the preliminary results of a new study of copper abundances in a large sample of metal-poor stars.

Affiliated with

Also associated with

No associations

Rating

Copper Abundances in 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 Copper Abundances in Metal-Poor Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Copper Abundances in Metal-Poor Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1421644