2021
DOI: 10.48550/arxiv.2105.14503
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

Merging timescale for supermassive black hole binary in interacting galaxy NGC 6240

Margarita Sobolenko,
Peter Berczik,
Rainer Spurzem

Abstract: Context. One of the main possible way of creating the supermassive black hole (SMBH) is a so call hierarchical merging scenario. Central SMBHs at the final phase of interacting and coalescing host-galaxies are observed as SMBH binary (SMBHB) candidates at different separations from hundreds of pc to mpc. Aims. Today one of the strongest SMBHB candidate is a ULIRG galaxy NGC 6240 which was X-ray spatially and spectroscopically resolved by Chandra. Dynamical calculation of central SMBHBs merging in a dense stell… Show more

Help me understand this report
View published versions

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals

citations
Cited by 0 publications
references
References 60 publications
(79 reference statements)
0
0
0
Order By: Relevance

No citations

Set email alert for when this publication receives citations?