Morphological and kinematic studies often
reveal unusual evidence of past interactions and minor
mergers, even in relatively normal spirals. |


Above: Three-dimensional distribution of galaxies in the
region of the Pisces-Perseus Supercluster (PPS). The upper panel shows the distribution
on the sky, with the density enhancement identified as the filamentary ridge of
the PPS outlined. The lower panel illustrates that the majority of the galaxies
in the ridge indeed lie at similar redshift, emphasizing that the PPS is an elongated
structure viewed nearly perpendicular to our line of sight. |