A close-pair binary in a distant triple supermassive black hole system.
Galaxies are believed to evolve through merging, which should lead to some hosting multiple supermassive black holes. There are four known triple black hole systems, with the closest black hole pair being 2.4 kiloparsecs apart (the third component in this system is at 3 kiloparsecs), which is far fr...
Main Authors: | Deane, R, Paragi, Z, Jarvis, M, Coriat, M, Bernardi, G, Fender, R, Frey, S, Heywood, I, Klöckner, H, Grainge, K, Rumsey, C |
---|---|
格式: | Journal article |
語言: | English |
出版: |
Nature Publishing Group
2014
|
相似書籍
-
Multiple supermassive black hole systems: SKA’s future leading role
由: Deane, R, et al.
出版: (2015) -
Investigating close binary supermassive black holes at high angular resolution
由: Kovačević A.
出版: (2021-01-01) -
High-energy signatures of binary supermassive black holes
由: Vila Gabriela S., et al.
出版: (2013-12-01) -
ASTRONOMICAL PLATE ARCHIVES AND SUPERMASSIVE BLACK HOLE BINARIES
由: René Hudec
出版: (2013-12-01) -
A binary system in the S cluster close to the supermassive black hole Sagittarius A*
由: Florian Peißker, et al.
出版: (2024-12-01)