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Beryllium and Boron abundances in population II starsThe scientific focus of this program was to undertake UV spectroscopic abundance analyses of extremely metal poor stars with attention to determining abundances of light elements such as beryllium and boron. The abundances are likely to reflect primordial abundances within the early galaxy and help to constrain models for early galactic nucleosynthesis. The general metal abundances of these stars are also important for understanding stellar evolution.
Document ID
19950026841
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Date Acquired
September 6, 2013
Publication Date
March 1, 1995
Subject Category
Astrophysics
Report/Patent Number
NAS 1.26:189434
RHPU-0429
NASA-CR-189434
Accession Number
95N33262
Funding Number(s)
CONTRACT_GRANT: NASA ORDER S-97228-E
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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