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Castro-Tirado, A J; Østgaard, N; Göǧüş, E; Sánchez-Gil, C; Pascual-Granado, J; Reglero, V; Mezentsev, A; Gabler, M; Marisaldi, M; Neubert, T; Budtz-Jørgensen, C; Lindanger, A; Sarria, D; Kuvvetli, I; Cerdá-Durán, P; Navarro-González, J; Font, J A; Zhang, B-B; Lund, N; Oxborrow, C A; Brandt, S; Caballero-García, M D; Carrasco-García, I M; Castellón, A; Castro Tirado, M A; Christiansen, F; Eyles, C J; Fernández-García, E; Genov, G; Guziy, S; Hu, Y-D; Nicuesa Guelbenzu, A; Pandey, S B; Peng, Z-K; Pérez Del Pulgar, C; Reina Terol, A J; Rodríguez, E; Sánchez-Ramírez, R; Sun, T; Ullaland, K; Yang, S
Nature (London), 12/2021, Letnik: 600, Številka: 7890Journal Article
Magnetars are strongly magnetized, isolated neutron stars with magnetic fields up to around 10 gauss, luminosities of approximately 10 -10 ergs per second and rotation periods of about 0.3-12.0 s. Very energetic giant flares from galactic magnetars (peak luminosities of 10 -10 ergs per second, lasting approximately 0.1 s) have been detected in hard X-rays and soft γ-rays , and only one has been detected from outside our galaxy . During such giant flares, quasi-periodic oscillations (QPOs) with low (less than 150 hertz) and high (greater than 500 hertz) frequencies have been observed , but their statistical significance has been questioned . High-frequency QPOs have been seen only during the tail phase of the flare . Here we report the observation of two broad QPOs at approximately 2,132 hertz and 4,250 hertz in the main peak of a giant γ-ray flare in the direction of the NGC 253 galaxy , disappearing after 3.5 milliseconds. The flare was detected on 15 April 2020 by the Atmosphere-Space Interactions Monitor instrument aboard the International Space Station, which was the only instrument that recorded the main burst phase (0.8-3.2 milliseconds) in the full energy range (50 × 10 to 40 × 10 electronvolts) without suffering from saturation effects such as deadtime and pile-up. Along with sudden spectral variations, these extremely high-frequency oscillations in the burst peak are a crucial component that will aid our understanding of magnetar giant flares.
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