The morphological type and derived physical parameters based on the SED modeling of the HCG galaxies.
Derived physical parameters based on the SED modeling of the interacting pair’s galaxy sample.
Distance to, virial radius, and morphology of the nearest neighbor, as well as “strength” of interaction for the HCG galaxies.
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