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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 4.

The Eddington timescale defined as the timescale that the debris mass fallback rate stays above the Eddington accretion rate. It is seen that Pop III star TDEs can stay super-Eddington for very long timescales (up to hundreds of years).

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