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The Light Curve of Wind-reprocessed Tidal Disruption Events

  • Authors: Brenna Mockler, David Khatami, Daniel Kasen, Xiaoshan Huang, Anthony L. Piro

Brenna Mockler et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 3.

The blue, green, and orange lines show the output SED using three different opacity prescriptions—bound-free (blue), bound-free + free–free (green), and bound-free + free–free + bound-bound (orange). All three also include electron scattering opacities. The top plot shows emission early on the rise at 7 days into the simulation, the middle plot shows emission at 49 days (near the optical/UV peak), and the bottom plot shows emission at 120 days, on the decline. The thin black solid lines show the source luminosity at these times, and the dotted black lines show example blackbody SEDs that match the emission relatively well in observable UV and optical bands, emphasizing the likelihood of underestimating the true luminosity when fitting blackbodies to observations. The shaded black, magenta, green, and red vertical regions represented the approximated band range of eRosita, Swift UV, and Palomar g and r bands.

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