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Estimation of the Neutron Star Mass and Radius of FRB 20240114A by Identification of Crustal Oscillations

  • Authors: Hajime Sotani, Z. Wadiasingh, C. Chirenti

Hajime Sotani et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

The ∼600 Hz candidate QPO frequencies observed in FRB 20240114A, compared with the first overtone excited in an NS model with 1.4M⊙, 12 km, and Ns/Nd = 1.

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