Online material
Table 4
The morphological type and derived physical parameters based on the SED modeling of the HCG galaxies.
Table 4
continued.
Table 5
Derived physical parameters based on the SED modeling of the interacting pair’s galaxy sample.
Table 6
Distance to, virial radius, and morphology of the nearest neighbor, as well as “strength” of interaction for the HCG galaxies.
Table 6
continued.
Table 7
Observed and predicted 60 μm and 100 μm IRAS fluxes for each group, as well as total HI, H2, stellar, and dynamical masses.
© ESO, 2011