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The Superluminous Transient ASASSN-15lh as a Tidal Disruption Event from a Kerr Black Hole

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Academic year: 2018

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Figure

Figure 1|Spectral sequence of ASASSN-15lh showing three spectroscopic phases.
Figure 2|The light curve evolution of ASASSN-15lh in the rest frame. The data
Figure 3|The evolution of the temperature, radius and luminosity of ASASSN-
Figure 4|The Hills mass MH as a function of SMBH spin a• for main sequence

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