  This paper briefly summarizes the search for astronomical sources of
high-energy neutrinos using the AMANDA-B10 detector. The complete data set from
1997 was analyzed. For E_mu>10 TeV, the detector exceeds 10,000 m^2 in
effective area between declinations of 25 and 90 degrees. Neutrinos generated
in the atmosphere by cosmic ray interactions were used to verify the overall
sensitivity of the detector. The absolute pointing accuracy and angular
resolution has been confirmed by the analysis of coincident events between the
SPASE air shower array and the AMANDA detector. Preliminary flux limits from
point source candidates are presented. For declinations larger than +45
degrees, our results compare favorably to existing limits for sources in the
Southern sky. We also present the current status of the searches for high
energy neutrino emission from diffusely distributed sources, GRBs, and WIMPs
from the center of the earth.
