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

When a star passes within the tidal radius of a supermassive black hole, it will be torn apart. For a star with the mass of the Sun (M ⊙) and a non-spinning black hole with a mass <10 8 M ⊙, the tidal radius lies outside the black hole event horizon2 and the disruption results in a luminous flare...

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Bibliographic Details
Main Authors: Leloudas, G., Fraser, M., Stone, N., van Velzen, S., Jonker, P., Arcavi, I., Fremling, C., Maund, J., Smartt, S., Krihler, T., Miller-Jones, James, Vreeswijk, P., Gal-Yam, A., Mazzali, P., De Cia, A., Howell, D., Inserra, C., Patat, F., Postigo, A., Yaron, O., Ashall, C., Bar, I., Campbell, H., Chen, T., Childress, M., Elias-Rosa, N., Harmanen, J., Hosseinzadeh, G., Johansson, J., Kangas, T., Kankare, E., Kim, S., Kuncarayakti, H., Lyman, J., Magee, M., Maguire, K., Malesani, D., Mattila, S., McCully, C., Nicholl, M., Prentice, S., Romero-Canizales, C., Schulze, S., Smith, K., Sollerman, J., Sullivan, M., Tucker, B., Valenti, S., Wheeler, J., Young, D.
Format: Journal Article
Published: NATURE PUBLISHING GROUP 2017
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/57814

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