Abstract:
As a result of studying the temporal structure of the light curve of the GRB 240825A $\gamma$-ray burst, recorded by Swift satellite equipment in the energy range of 15 – 350 keV, for the presence of quasi-periodic components, oscillations with periods of 0.384, 0.768, 1.224 and 1.536 s were detected. Moreover the oscillation with a period of 1.536 s turned out to be modulated with the same period. Assuming that the modulation is caused by the relativistic Doppler effect during the orbital motion of the emitting object around a more massive central body, the orbital parameters of the emitting object and the mass of the central body were calculated in the classical approximation.
Keywords:periodogramanalysis, quasiperiodicities, model – amplitude-frequency modulation.