Boron in Main Sequence STARS-CYC3HIGH

Details Boron in Main Sequence STARS-CYC3HIGH Boron in Main Sequence STARS-CYC3HIGH

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4840l&link_type=abstract

HST Proposal ID #4840

Physics

Hst Proposal Id #4840

Scientific paper

Boron abundances have been obtained for a sample of Pop. I and Pop. II stars from GHRS grating/echelle spectra of the BI resonance lines at 2497 A. Stars to be observed in Cycle 3 include Procyon and high galactic latitude early type stars. Boron will A B I line at 2089A will be observed in Procyon in order to measure the 11B/10B ratio. In the high latitude B stars, Boron will be sought from the B II doublet at 1362A. A second region at 1305A will provide profiles of SiIII lines; a SiIII line is blended with the B II line. Boron will provide a new clue to origins of these young solar-metallicity massive stars in the halo.

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