Physics
Scientific paper
Jul 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8770b&link_type=abstract
HST Proposal ID #8770
Physics
Hst Proposal Id #8770
Scientific paper
In spite of several HST cycles of boron abundance determinations, we do not know the true, ambient, present-day abundance of B. Only two stars {with undepleted Li and Be} have been observed to derive the Population I true B abundance. Past cycles have focused on {1} halo stars with low metallicity and {2} solar-type stars with Li and/or Be deficiencies. In this study we wish to determine stellar abundances of boron, measured from the B I 2497 Angstrom line from STIS echelle spectra, of main sequence F-G stars that have retained their full initial abundances of boron. Our target stars are those for which ground-based observations show that beryllium is undepleted. These new abundances will map evolution of the boron abundance in the Galactic disk in the metallicity range from one-third solar up to solar. Then the B, and previously determined Li and Be abundances, will be used to improve understanding of the nucleosynthesis of B. In particular, we will be able to assess the relative contributions from cosmic ray-induced spallation vs neutrino-induced spallation in Type II SN, that are predicted to synthesize B {as ^11B} but not Be. Since the former process is the only identified site of Be synthesis, the B/Be ratio can be used to resolve the contributions of neutrino and cosmic ray induced spallation.
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