Аннотация:VV 126 has been investigated on spectrograms taken with the 6-m telescope. This object is a system of two or more distorted giant galaxies having a peculiar velocity field and emission knots representing giant H II regions, or superassociations. If the system is stable its total mass should be equal to about 10 to the 11th solar masses. The relative emission-line intensities are similar to those observed for H II regions in the spiral structure of ordinary galaxies.