Abell 400

Source: Wikipedia, the free encyclopedia.
keV)[1]
See also: Galaxy group, Galaxy cluster, List of galaxy groups and clusters

Abell 400 is a

) spiraling towards merger.

These two supermassive black holes are contained in NGC 1128. The galaxy, microwave radio jets, multi-million degree X-ray producing gas and resultant radio source is known as 3C 75. X-ray source 2A 0252+060 (1H 0253+058, XRS 02522+060) may be some additional or other portion of Abell 400.[3]

The black holes are an estimated 25,000 light years apart, and thus will take millions of years to collide. Should the two supermassive black holes merge, they will form a single super-supermassive black hole.[4]

Gallery

  • wider view of Abell 400 with PanSTARRS
  • Two supermassive black holes 3C 75 spiraling towards merger near the center of NGC 1128, some 25,000 light years away from each other.

See also

References

  1. ^ a b c d "NED results for object ABELL 0400". NASA/IPAC Extragalactic Database (NED). Retrieved March 15, 2012.
  2. ^
    ISSN 0067-0049
    . Retrieved March 12, 2012.
  3. .
  4. ^ "Chandra :: Photo Album :: 3C 75 in Abell 400 :: 06 Apr 06". chandra.harvard.edu. Retrieved 2019-02-16.

External links