  In this talk I will first give a summary of the observations of expected
Galactic TeV gamma-ray sources with the HEGRA CT-Sytem since the Kruger Park
Workshop in 1997. Then I will go into some detail regarding the observations of
Supernova Remnants (SNRs), especially those of Tycho's SNR and of Cas A. The
emphasis will not be on all aspects of these published data. I will rather
review the selection of these observational targets, and discuss some of the
physical implications of the results.
