Profiles of Lyman\alpha\ Emission Lines
  We present the results of the observations of the Ly\alpha\ line profiles of
91 emission-line galaxies at z=3.1 with the spectral resolution of
\lambda/\delta\lambda (FWHM) = 1700, or 180 km/s. A significant fraction, ~50%
of the observed objects show the characteristic double peaks in their Ly\alpha
profile. The red peak is much stronger than the blue one for most of the cases.
The red peaks themselves also show weak but significant asymmetry and their
widths are correlated with the velocity separation of the red and the blue
peaks, which implies that the peaks are not isolated multiple components with
different velocities but the parts of the single line which is modified by the
absorption and/or scattering by the associated neutral hydrogen gas. The
characteristic profile can be naturally explained by the scattering in the
expanding shell of neutral hydrogen surrounding the Ly\alpha\ emitting region
while the attenuation by the inter-galactic medium should also be considered.
Our results suggest that the star-formation in these Ly\alpha\ emitters are
dominated by the young burst-like events which produce the intrinsic Ly\alpha\
emission as well as the gas outflow.
