Very-high-frequency Oscillations in the Main Peak of a Magnetar Giant Flare.

Magnetars are strongly magnetized, isolated neutron stars 1 – 3 with magnetic fields up to around 10 15 gauss, luminosities of approximately 10 31 –10 36 ergs per second and rotation periods of about 0.3–12.0 s. Very energetic giant flares from galactic magnetars (peak luminosities of 10 44 –10 47 ergs per second, lasting approximately 0.1 s) have been detected in hard X-rays and soft γ-rays 4 , and only one has been detected from outside our galaxy 5 . During such giant flares, quasi-periodic oscillations (QPOs) with low (less than 150 hertz) and high (greater than 500 hertz) frequencies have been observed 6 – 9 , but their statistical significance has been questioned 10 . High-frequency QPOs have been seen only during the tail phase of the flare 9 . 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 11 in the direction of the NGC 253 galaxy 12 – 17 , disappearing after 3.5 milliseconds. The flare was detected on 15 April 2020 by the Atmosphere–Space Interactions Monitor instrument 18 , 19 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 3 to 40 × 10 6 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.