A Chemical Abundance Survey of Solar Neighborhood, Solar-Like Stars.

Details A Chemical Abundance Survey of Solar Neighborhood, Solar-Like Stars. A Chemical Abundance Survey of Solar Neighborhood, Solar-Like Stars.

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phdt........84m&link_type=abstract

Thesis (PH.D.)--GEORGIA STATE UNIVERSITY, 1990.Source: Dissertation Abstracts International, Volume: 51-08, Section: B, page: 38

Physics

Scientific paper

A high precision differential chemical abundance analysis (with respect to the Sun) has been carried out for the near solar-like stars HR 483, HR 3881, HR 4277, and HR 5459. The maximum error in the determinations is 0.1 dex. The literatures of galactic chemical evolution, and of stellar nucleosynthesis have been surveyed to provide the context for the study. Using the high precision abundance analysis performed for these stars, suggestions are made as to which types of stellar events prior to the formation of these stars led to their chemical deviations from the Sun. In this way, the chemical evolution of this part of the Galaxy is explored.

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