  We have determined beryllium abundances for 25 metal-poor stars based on the
high resolution and high signal-to-noise ratio spectra from the VLT/UVES
database. Our results confirm that Be abundances increase with Fe, supporting
the global enrichment of Be in the Galaxy. Oxygen abundances based on [O I]
forbidden line implies a linear relation with a slope close to one for the Be
vs. O trend, which indicates that Be is probably produced in a primary process.
Some strong evidences are found for the intrinsic dispersion of Be abundances
at a given metallicity. The deviation of HD132475 and HD126681 from the general
Be vs. Fe and Be vs. O trend favours the predictions of the superbubble model,
though the possibility that such dispersion originates from the inhomogeneous
enrichment in Fe and O of the protogalactic gas cannot be excluded.
