Abstract
When a star passes within the tidal radius of a supermassive black hole,
it will be torn apart1. For a star with the mass of the Sun
(M ⊙) and a non-spinning black hole with a mass
108 M ⊙ 12,13, a
star with the same mass as the Sun could be disrupted outside the event
horizon if the black hole were spinning rapidly14. The rapid
spin and high black hole mass can explain the high luminosity of this
event.
| Original language | English |
|---|---|
| Article number | 0002 |
| Journal | Nature Astronomy |
| Volume | 1 |
| DOIs | |
| Publication status | Published - 12 Dec 2016 |
Fingerprint
Dive into the research topics of 'The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole'. Together they form a unique fingerprint.Student theses
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Unravelling the nature of hydrogen-poor thermonuclear supernovae
Magee, M. (Author), Smartt, S. (Supervisor) & Sim, S. (Supervisor), Jul 2019Student thesis: Doctoral Thesis › Doctor of Philosophy
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