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Binary Black Hole in 3C 75
http://antwrp.gsfc.nasa.gov/apod/ap100314.html

Explanation:
What's happening in the middle of this massive galaxy? There, two bright 
sources at the center of this composite x-ray (blue)/radio (pink) image 
are thought to be co-orbiting supermassive black holes powering the 
giant radio source 3C 75. Surrounded by multimillion degree x-ray 
emitting gas, and blasting out jets of relativistic particles the 
supermassive black holes are separated by 25,000 light-years. At the 
cores of two merging galaxies in the Abell 400 galaxy cluster they are 
some 300 million light-years away. Astronomers conclude that these two 
supermassive black holes are bound together by gravity in a binary 
system in part because the jets' consistent swept back appearance is 
most likely due to their common motion as they speed through the hot 
cluster gas at 1200 kilometers per second. Such spectacular cosmic 
mergers are thought to be common in crowded galaxy cluster environments 
in the distant universe. In their final stages the mergers are expected 
to be intense sources of gravitational waves.


3C75 - Central Galaxy em Abell 400
http://images.nrao.edu/object/index.php?id=30


Merging Galaxies Create a Binary Quasar
http://www.youtube.com/watch?v=4tmsK5kAyNc


Descrição:
Astronomers have found the first clear evidence of a binary quasar 
within a pair of actively merging galaxies. Quasars are the extremely 
bright centers of galaxies surrounding super-massive black holes, and 
binary quasars are pairs of quasars bound together by gravity. Binary 
quasars, like other quasars, are thought to be the product of galaxy 
mergers. Until now, however, binary quasars have not been seen in 
galaxies that are unambiguously in the act of merging. But images of a 
new binary quasar from the Carnegie Institutions Magellan telescope in 
Chile show two distinct galaxies with tails produced by tidal forces 
from their mutual gravitational attraction.

Cont...

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