- Abstract:
-
We explore the rates of tidal disruption events (TDEs) of stars by supermassive black holes (SBHs) in galactic nuclei formed in mergers followed by a formation and coalescence of a binary SBH. Such systems initially have a deficit of stars on low-angular-momentum orbits caused by the slingshot process during the binary SBH stage, which tends to reduce the flux of stars into the SBH compared to the steady-state value. On the other hand, a newly formed galactic nucleus has a non-spherical shape...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's Version
- Files:
-
-
(pdf, 440.8kb)
-
- Publisher copy:
- 10.3847/0004-637X/831/1/84
-
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- Funding agency for:
- Vasiliev, Euegene
- Publisher:
- American Astronomical Society Publisher's website
- Journal:
- The Astrophysical Journal Journal website
- Volume:
- 831
- Issue:
- 1
- Pages:
- 1-8
- Publication date:
- 2016-10-28
- Acceptance date:
- 2016-08-17
- DOI:
- EISSN:
-
1538-4357
- ISSN:
-
0004-637X
- Pubs id:
-
pubs:641558
- URN:
-
uri:a3ef8994-b35d-47bc-9df0-c3a01012c007
- UUID:
-
uuid:a3ef8994-b35d-47bc-9df0-c3a01012c007
- Local pid:
- pubs:641558
- Copyright holder:
- © 2016. The American Astronomical Society. All rights reserved.
- Copyright date:
- 2016
- Notes:
- © 2016. The American Astronomical Society. All rights reserved. This is the Publisher's Version of the article. The final version is available online from Tne American Astronomical Society at: 10.3847/0004-637X/831/1/84
Journal article
Tidal disruption rates in non-spherical galactic nuclei formed by galaxy mergers
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