Boron in Main Sequence Stars Cycle 0 Observations

Details Boron in Main Sequence Stars Cycle 0 Observations Boron in Main Sequence Stars Cycle 0 Observations

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1064l&link_type=abstract

HST Proposal ID #1064

Physics

Hst Proposal Id #1064

Scientific paper

Boron abundances will be obtained for a sample of Pop. I and Pop. II main sequence stars from HRS spectra of the BI resonance lines at 2497 A. Stars to be observed include - Noraml F dwarfs including stars showing the unexplained large deficiencies of Li and Be. Boron will provide a new clue to the processes depleting Li and Be. - Old Disk and Halo Dwarfs with metal abundances in the range [Fe/H] ~ -0.3 to -2.4. These observations will reveal the evolution of the boron abundance with overall metal abundance and age.

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