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...
Autores principales: | Deane, R, Paragi, Z, Jarvis, M, Coriat, M, Bernardi, G, Fender, R, Frey, S, Heywood, I, Klöckner, H, Grainge, K, Rumsey, C |
---|---|
Formato: | Journal article |
Lenguaje: | English |
Publicado: |
Nature Publishing Group
2014
|
Ejemplares similares
-
Multiple supermassive black hole systems: SKA’s future leading role
por: Deane, R, et al.
Publicado: (2015) -
Investigating close binary supermassive black holes at high angular resolution
por: Kovačević A.
Publicado: (2021-01-01) -
High-energy signatures of binary supermassive black holes
por: Vila Gabriela S., et al.
Publicado: (2013-12-01) -
ASTRONOMICAL PLATE ARCHIVES AND SUPERMASSIVE BLACK HOLE BINARIES
por: René Hudec
Publicado: (2013-12-01) -
A binary system in the S cluster close to the supermassive black hole Sagittarius A*
por: Florian Peißker, et al.
Publicado: (2024-12-01)