General Caption: Images of the galaxy cluster the Coma Cluster.
Follow-up observations showed that many of these astronomical objects are dwarf galaxies belonging to the Coma Cluster. Two large elliptical galaxy, NGC 4889 (a cD galaxy (AKA supergiant elliptical galaxy) and NGC 4874 (a giant elliptical galaxy), dominate the central region. The mosaic combines visible data from the Sloan Digital Sky Survey (SDSS) (color coded blue) with long- and short-wavelength infrared views (red and green, respectively) from NASA's Spitzer Space Telescope.
The Coma Cluster is a RICH galaxy cluster (more than 1000 identified galaxies) in the constellation Coma Berenices (Berenice's Hair) (the only IAU designated constellation named for a historical person or at least their hair: Queen Berenice II of Egypt (267/266--221 BCE)).
It is located at distance 102.975 Mpc = 336 Mly (for Hubble constant = 70.5 (km/s)/Mpc) and at cosmological redshift z = 0.0231 or redshift velocity = 6925 km/s.
Its velocity dispersion (σ) ∼ 1000 km/s. Its size scale is ∼ 14 Mpc.????
The foreground stars in the mosaic (which combines images from two CCD cameras) have both 4 points nad 6 points which means one camera was held up by 4 arms and the other by 6 arms.
The elliptical galaxies
NGC 4889
and NGC 4874
from the
mosaic above can be located.
NGC stands for
New General Catalogue (NGC)
and
IC for
Index Catalogue (IC).