- Table 1:
- Table 3:
Classification of the DPOSS II compact groups and neighbouring
large scale structures. n represents all galaxies which fulfilled the
velocity criteria, irrespective of the original catalogue of group galaxies, while the number quoted
in parentheses is the number of concordant galaxies that were originally part of the
DPOSS catalog. When a (2+2) is given for n (members), it means that the
candidate group is composed of two concordant pairs of galaxies.
- Table 4:
Morphological classification of the member galaxies for groups of class A and B.
is the morphogical type of the group as defined by the percentage of galaxies
- Table 5:
Group dynamical properties.
expressed in logarithmic values; mass,
luminosity, and mass-to-light ratio are given in solar units. The symbols follow Hickson et al. (1992).
- Table 2:
Observed compact groups candidates from the DPOSS survey. Column 5 lists
the kind of spectrum for each galaxy: abs means a spectrum which is dominated by absorption lines;
em means a spectrum dominated by emission lines and mix a spectrum
where both emission and absorption lines are present. The most significant emission lines
have been listed for the observed galaxies.