An Observational Perspective on Some Aspects of Early Stellar Nucleosynthesis

Details An Observational Perspective on Some Aspects of Early Stellar Nucleosynthesis An Observational Perspective on Some Aspects of Early Stellar Nucleosynthesis

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990...90s&link_type=abstract

FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 90-103 (2008).

Computer Science

3

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Star Formation, Population Iii Stars, Abundances, Chemical Composition, Population Ii Stars

Scientific paper

Some basic abundance results for low metallicity stars that were formed in the early days of the Milky Way Galaxy are summarized. Discussion is centered on two nucleosynthetic groups: the light α elements (Mg, Si, and Ca), and the neutron-capture elements (those heavier than the Fe group, atomic numbers greater than 30). Emphasis is placed on the present state of stellar spectroscopic and atomic transition data.

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