Not exact matches
The estimates of the number of dwarf
irregulars and dwarf ellipticals are based on the proportions of these types of
galaxies in
nearby groups.
Pictures from the Hubble Space Telescope of very distant
galaxies show more distorted shapes, bent spiral arms, and
irregular fragments than in
nearby galaxies (seen in a more recent stage of their evolution).
«The beauty of this is that dwarf
irregulars are the most numerous type of
galaxy, and many, like IC 10, are relatively
nearby.