  In the course of our on-going search for serendipitous high-redshift LyA
emission in deep archival Keck spectra, we discovered two LyA emission line
candidates in a moderate dispersion ($\lambda/{\Delta \lambda} +~ 1200$)
spectrogram. Both lines have high equivalent width (EW_{obs}>= 450A), low
velocity dispersions ($\sigma_v ~ 60 km/s), and deconvolved effective radii
$r_e ~ 1.0 h_{50}^{-1}$ kpc. Their sizes and luminosities are suggestive of the
primeval galaxy model of Lin & Murray (1992), based on the self-similar
collapse of an isothermal sphere. We argue that the line emission is LyA, and
it is stellar in origin. The sources are consistent with being primeval.
