Boron in the very metal-poor star BD 13 3442 ?

The Goddard High Resolution Spectrograph (GHRS) of the Hubble Space Telescope (HST)has been used to observe the boron 2500 ˚ A region of BD 13 3442. At a metallicity of (Fe/H)= 3.00 this is the most metal-poor star ever observed for B. Nearly 26 hours of exposure time resulted in a detection. Spectrum synthesis using the latest Kurucz model atmospheres yields an LTE boron abundance of log �(B) =+ 0.01 ± 0.20. This value is consistent with the linear relation of slope �1.0 between log �(BLTE) and (Fe/H) found for 10 halo and disk stars by Duncan et al. (1997). Using the NLTE correction of Kiselman & Carlsson (1996), the NLTE boron abundance is log �(B) =+ 0 .93 ± 0.20. This is also consistent with the NLTE relation determined by Duncan et al. (1997) where the slope of log �(BNLTE) vs. (Fe/H) is �0.7. These data support a model in which most production of B and Be comes from the spallation of energetic C and O nuclei onto protons and He nuclei, probably in the vicinity of massive supernovae in star-forming regions, rather than the spallation of cosmic ray protons and alpha particles onto CNO nuclei in the general interstellar medium.