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The TDE Population from First-principles Models of Stellar Disruption and Debris Dynamics

  • Authors: Tsvi Piran, Julian Krolik, Taeho Ryu

Tsvi Piran et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 4.

The total (full + partial) event rate density in the ﹩\mathrm{log}{M}_{{\rm{BH}}}\times \mathrm{log}{L}_{{\rm{peak}}}﹩ plane for flux-limited samples. Both panels assume that the stellar mass function is proportional to a Salpeter IMF, but in the left panel αBH = −0.5 and in the right panel αBH = +0.5. Rates (in arbitrary units) are shown on a linear scale calibrated by the color bar.

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