This paper presents two galaxy samples, respectively in a high and in
a low local density environments, that were generated from the SSRS ca
talog using objective criteria. A preliminary comparison of physical p
roperties in these two samples reveals that galaxies in high-density e
nvironments tend to be under a higher starbursting activity, have a de
ficiency of the neutral hydrogen content, present a higher fractional
Seyfert population and a higher fraction of barred spirals as well. Th
e present samples are intended to be used in future spectroscopic obse
rvations for more detailed investigation.