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- W2377135394 abstract "In this paper, we discussed the time profiles and energy spectra of cosmic γ-ray event on 5 March 1979. we obtained: (1)The energy spectrum in burst (0~s.3) can be fitted by a thermal bremsstrahlung with KT～50 Kev, a bremsstrahlung of relativistic electrons with equivalent Lorentz factor γ=3.3 and a broad line at 430 Key; (2) The average spectrum in pulsating phase fits with a bremsstrahlung of thermal electrons with KT～40 Kev; (3) The time profile in pulsating phase can be fitted by bremsstrahlung radiation of the radiative region which are cooling with time. Based on these results we proposed a morphological model as follows: Because of some reason, a great deal of matter suddenly injects onto the surface at magnetic poles of a neutron star. The gravitational energy of electrons transforms into radiation in phase through bremsstrahlung of electrons. At first the gravitational energy of protons transforms into heat in radiative region and then the radiative region gives radiation in pulsating phase by bremsstrahlung of thermal electrons." @default.
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- W2377135394 date "1981-09-01" @default.
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- W2377135394 title "A MODEL OF COSMIC GAMMA-RAY BURST EVENT ON 5 MARCH 1979" @default.
- W2377135394 hasPublicationYear "1981" @default.
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