Journal article
Effect of mass-loss due to stellar winds on the formation of supermassive black hole seeds in dense nuclear star clusters
- Abstract:
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The observations of high-redshifts quasars at z ≳ 6 have revealed that supermassive black holes (SMBHs) of mass ∼109M⊙∼109M⊙ were already in place within the first ∼Gyr after the big bang. Supermassive stars (SMSs) with masses 103−5M⊙103−5M⊙ are potential seeds for these observed SMBHs. A possible formation channel of these SMSs is the interplay of gas accretion and runaway stellar collisions inside dense nuclear star clusters (NSCs). However, mass-loss due to stellar winds could be an import...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Version of record, 746.0KB)
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- Publisher copy:
- 10.1093/mnras/stab1428
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Authors
Bibliographic Details
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 505
- Issue:
- 2
- Pages:
- 2186-2194
- Publication date:
- 2021-05-19
- Acceptance date:
- 2021-05-13
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
Item Description
- Language:
- English
- Keywords:
- Pubs id:
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1188026
- Local pid:
- pubs:1188026
- Deposit date:
- 2021-08-13
Terms of use
- Copyright holder:
- Das et al.
- Copyright date:
- 2021
- Rights statement:
- © 2021 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.
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