Most clusters in the universe today are dominated
by giant elliptical galaxies in which the dust and gas has already been formed into stars.
Not exact matches
Some
ellipticals are present in the central part of the cluster including a
giant elliptical at the center (M87) that has become so large
by gobbling up nearby galaxies that were attracted
by its enormous gravity.
The research team led
by Satoru Iguchi, Associate Professor of NAOJ, succeeded in observing a very close binary black hole in the center of 3C66B (a
giant elliptical galaxy within the cluster A347) just before its black hole merger.
Detection of the spiral's dust in a bi-symmetric structure provides strong evidence of its position deep inside the
giant elliptical host while the vast amounts of radio, visual, and x-ray emissions are a result of the energy released
by this continuing galactic merger (or «consumption» of a satellite galaxy).
On June 16, 2010, the Hubble Heritage Project released a very detailed, composite image of the dark lanes of dust crisscrossing the
giant elliptical galaxy Centaurus A. Taken on July 10, 2010 with the Hubble Space Telescope's Wide Field Camera 3, the panchromatic image of ultraviolet through near - infrared wavelengths shows new details such as bluish clusters of young massive stars and reddish gas nebulae undergoing star birth normally obscured
by dust.