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Detecting Population III Stars through Tidal Disruption Events in the Era of JWST and Roman

Authors: Rudrani Kar Chowdhury, Janet N. Y. Chang, Lixin Dai, Priyamvada Natarajan

Rudrani Kar Chowdhury et al 2024 The Astrophysical Journal Letters 966 .

Provider: AAS Journals

Caption: Figure 5.

The time that the photosphere transits from expansion to recession (t _edge) as a function of M _BH for various types of stars. The color scheme is the same as Figure 3. t _edge is longer for the Pop III stars compared to solar-type stars.

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