Compact groups of galaxies are fruitful laboratories to study such pro
cesses as dynamical friction, tidal interaction, collision, and galaxy
mergers. The largest survey of compact galaxy groups is the one of Sh
akhbazian, Petrosian, Baier, Tiersch. A programme to evaluate photomet
rical properties of the galaxies in the Shakhbazian groups has been st
arted using the COSMOS/UKST catalogue of the Southern sky with delta l
ess-than-or-equal-to +2-degrees-30'. About a quarter of the Shakhbazia
n groups lie south of this declination limit. A list of 24 groups (Shk
h 21, 24, 27, 30, 32, 33, 35, 81, 82, 83, 140, 141, 143, 144, 145, 146
, 147, 148, 151, 152, 154, 261, 262, 263) is our first result.