Galactic Evolution of Boron

Details Galactic Evolution of Boron Galactic Evolution of Boron

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...186.5001d&link_type=abstract

American Astronomical Society, 186th AAS Meeting, #50.01; Bulletin of the American Astronomical Society, Vol. 27, p.883

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations of the BI 2500 Angstroms line have been obtained with the Goddard High Resolution Spectrograph of the Hubble Space Telescope in 6 intermediate metal poor stars. Metallicities of the stars range from [Fe/H] = -0.35 to -2.5. The latest Kurucz model atmospheres and a single optimized line list are used to produce synthetic spectra and determine the B abundance in each star. The evolution of the galactic B abundance over this range of metallicity is compared to predictions of theoretical models for the evolution of light elements in the galaxy.

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