  We construct a galaxy groups catalogue from the public 100K data release of
the 2dF galaxy redshift survey. The group identification is carried out using a
slightly modified version of the group finding algorithm developed by Huchra &
Geller. Several tests using mock catalogues allow us to find the optimal
conditions to increase the reliability of the final group sample. A minimum
number of 4 members, an outer number density enhancement of 80 and a linking
radial cutoff of $200 km sec^{-1}$, are the best obtained values from the
analysis. Using these parameters, approximately 90% of groups identified in
real space have a redshift space counterpart. On the other hand the level of
contamination in redshift space reaches to 30 % including a $\sim 6%$ of
artificial groups and $\sim 24%$ of groups associated with binaries or triplets
in real space. The final sample comprise 2209 galaxy groups covering the sky
region described by Colless et al. spanning over the redshift range of $0.003
\leq z \leq 0.25$ with a mean redshift of 0.1.
