We present spectrophotometry of a sample of 26 Southern binary galaxie
s 17 pairs were confirmed to be physically associated with typical sep
aration of 136 h(-1) kpc. Pairs with velocity difference Delta v great
er than or equal to 600 km s(-1) are probably not physically bound. A
comparison with field galaxies suggests that galaxies in pairs tend to
have a younger population probably stimulated by tidal interaction. N
o correlation between the young population and projected separation wa
s found.