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ASASSN-15lh: a TDE about a maximally rotating 109 M⊙ black hole

Abstract:

We model the light curves of the novel and extremely luminous transient ASASSN-15lh at nine different frequencies, from infrared to ultraviolet photon energies, as an evolving relativistic disc produced in the aftermath of a tidal disruption event (TDE). Good fits to all nine light curves are simultaneously obtained when Macc ≃ 0.07 M⊙ is accreted on to a black hole of mass M ≃ 109 M⊙ and near-maximal rotation a/rg = 0.99. The best-fitting black hole mass is consistent with a number of existi...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnrasl/slaa105

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Wadham College
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0002-0934-1501
Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society: Letters More from this journal
Volume:
497
Issue:
1
Pages:
L13–L18
Publication date:
2020-06-03
Acceptance date:
2020-05-28
DOI:
EISSN:
1745-3933
ISSN:
1745-3925
Language:
English
Keywords:
Pubs id:
1111593
Local pid:
pubs:1111593
Deposit date:
2020-06-11

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