The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole

G. Leloudas; M. Fraser; N. C. Stone; S. van Velzen; P.G. Jonker; I. Arcavi; C. Fremling; J. R. Maund; S. J. Smartt; T. Krìhler; J. C. A. Miller-Jones; P.M. Vreeswijk; A. Gal-Yam; Paolo A. Mazzali; A. De Cia; D. A. Howell; C. Inserra; F. Patat; A. de Ugarte Postigo; Ofer Yaron; C. Ashall; I. Bar; H. Campbell; T.-W. Chen; M. Childress; N. Elias-Rosa; J. Harmanen; G. Hosseinzadeh; J. Johansson; T. Kangas; E. Kankare; S. Kim; H. Kuncarayakti; J. D. Lyman; M. R. Magee; Kate Maguire; D. Malesani; S. Mattila; C. V. McCully; M. Nicholl; S. Prentice; C. Romero-Cañizales; S. Schulze; K. W. Smith; J. Sollerman; M. Sullivan; Brad E. Tucker; S. Valenti; J. C. Wheeler; D. R. Young

doi:10.1038/s41550-016-0002

The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole

G. Leloudas, M. Fraser, N. C. Stone, S. van Velzen, P.G. Jonker, I. Arcavi, C. Fremling, J. R. Maund, S. J. Smartt, T. Krìhler, J. C. A. Miller-Jones, P.M. Vreeswijk, A. Gal-Yam, Paolo A. Mazzali, A. De Cia, D. A. Howell, C. Inserra, F. Patat, A. de Ugarte Postigo, Ofer YaronC. Ashall, I. Bar, H. Campbell, T.-W. Chen, M. Childress, N. Elias-Rosa, J. Harmanen, G. Hosseinzadeh, J. Johansson, T. Kangas, E. Kankare, S. Kim, H. Kuncarayakti, J. D. Lyman, M. R. Magee, Kate Maguire, D. Malesani, S. Mattila, C. V. McCully, M. Nicholl, S. Prentice, C. Romero-Cañizales, S. Schulze, K. W. Smith, J. Sollerman, M. Sullivan, Brad E. Tucker, S. Valenti, J. C. Wheeler, D. R. Young

School of Mathematics and Physics

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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	https://doi.org/10.1038/s41550-016-0002
Publication status	Published - 12 Dec 2016

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The Superluminous Transient ASASSN-15lh as a Tidal Disruption Event from a Kerr Black Hole
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Accepted author manuscript, 3.36 MBLicence: Unspecified

http://adsabs.harvard.edu/abs/2016NatAs...1E...2L

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Leloudas, G., Fraser, M., Stone, N. C., van Velzen, S., Jonker, P. G., Arcavi, I., Fremling, C., Maund, J. R., Smartt, S. J., Krìhler, T., Miller-Jones, J. C. A., Vreeswijk, P. M., Gal-Yam, A., Mazzali, P. A., De Cia, A., Howell, D. A., Inserra, C., Patat, F., de Ugarte Postigo, A., ... Young, D. R. (2016). The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole. Nature Astronomy, 1, Article 0002. https://doi.org/10.1038/s41550-016-0002

@article{ed80d3e50d6041afaed6c5ae5282f657,

title = "The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole",

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.",

author = "G. Leloudas and M. Fraser and Stone, {N. C.} and {van Velzen}, S. and P.G. Jonker and I. Arcavi and C. Fremling and Maund, {J. R.} and Smartt, {S. J.} and T. Kr{\`i}hler and Miller-Jones, {J. C. A.} and P.M. Vreeswijk and A. Gal-Yam and Mazzali, {Paolo A.} and {De Cia}, A. and Howell, {D. A.} and C. Inserra and F. Patat and {de Ugarte Postigo}, A. and Ofer Yaron and C. Ashall and I. Bar and H. Campbell and T.-W. Chen and M. Childress and N. Elias-Rosa and J. Harmanen and G. Hosseinzadeh and J. Johansson and T. Kangas and E. Kankare and S. Kim and H. Kuncarayakti and Lyman, {J. D.} and Magee, {M. R.} and Kate Maguire and D. Malesani and S. Mattila and McCully, {C. V.} and M. Nicholl and S. Prentice and C. Romero-Ca{\~n}izales and S. Schulze and Smith, {K. W.} and J. Sollerman and M. Sullivan and {E. Tucker}, Brad and S. Valenti and Wheeler, {J. C.} and Young, {D. R.}",

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Leloudas, G, Fraser, M, Stone, NC, van Velzen, S, Jonker, PG, Arcavi, I, Fremling, C, Maund, JR, Smartt, SJ, Krìhler, T, Miller-Jones, JCA, Vreeswijk, PM, Gal-Yam, A, Mazzali, PA, De Cia, A, Howell, DA, Inserra, C, Patat, F, de Ugarte Postigo, A, Yaron, O, Ashall, C, Bar, I, Campbell, H, Chen, T-W, Childress, M, Elias-Rosa, N, Harmanen, J, Hosseinzadeh, G, Johansson, J, Kangas, T, Kankare, E, Kim, S, Kuncarayakti, H, Lyman, JD, Magee, MR, Maguire, K, Malesani, D, Mattila, S, McCully, CV, Nicholl, M, Prentice, S, Romero-Cañizales, C, Schulze, S, Smith, KW, Sollerman, J, Sullivan, M, E. Tucker, B, Valenti, S, Wheeler, JC & Young, DR 2016, 'The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole', Nature Astronomy, vol. 1, 0002. https://doi.org/10.1038/s41550-016-0002

TY - JOUR

T1 - The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole

AU - Leloudas, G.

AU - Fraser, M.

AU - Stone, N. C.

AU - van Velzen, S.

AU - Jonker, P.G.

AU - Arcavi, I.

AU - Fremling, C.

AU - Maund, J. R.

AU - Smartt, S. J.

AU - Krìhler, T.

AU - Miller-Jones, J. C. A.

AU - Vreeswijk, P.M.

AU - Gal-Yam, A.

AU - Mazzali, Paolo A.

AU - De Cia, A.

AU - Howell, D. A.

AU - Inserra, C.

AU - Patat, F.

AU - de Ugarte Postigo, A.

AU - Yaron, Ofer

AU - Ashall, C.

AU - Bar, I.

AU - Campbell, H.

AU - Chen, T.-W.

AU - Childress, M.

AU - Elias-Rosa, N.

AU - Harmanen, J.

AU - Hosseinzadeh, G.

AU - Johansson, J.

AU - Kangas, T.

AU - Kankare, E.

AU - Kim, S.

AU - Kuncarayakti, H.

AU - Lyman, J. D.

AU - Magee, M. R.

AU - Maguire, Kate

AU - Malesani, D.

AU - Mattila, S.

AU - McCully, C. V.

AU - Nicholl, M.

AU - Prentice, S.

AU - Romero-Cañizales, C.

AU - Schulze, S.

AU - Smith, K. W.

AU - Sollerman, J.

AU - Sullivan, M.

AU - E. Tucker, Brad

AU - Valenti, S.

AU - Wheeler, J. C.

AU - Young, D. R.

PY - 2016/12/12

Y1 - 2016/12/12

N2 - 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.

AB - 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.

UR - https://arxiv.org/abs/1609.02927

U2 - 10.1038/s41550-016-0002

DO - 10.1038/s41550-016-0002

M3 - Article

VL - 1

JO - Nature Astronomy

JF - Nature Astronomy

M1 - 0002

ER -

The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole

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The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole

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