On 5 March 1979, an intense burst of hard X-rays and γ-rays was recorded, Qu and his collegues analysed its light curve and energy spectrum, provided detailed explanation of the observational data using the mechanism of bremsstrahlung and Kruskal-Schwarzschild instability.
On 5 March 1979, an intense burst of hard X-rays and γ-rays was recorded, Qu and his collegues analysed its light curve and energy spectrum. They created a model for neutron star binary system, provided detailed explanation of the observational data using the mechanism of bremsstrahlung and Kruskal-Schwarzschild instability.