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- W2463725397 abstract "The relationship between the pulse FWHM (full-widths at half maximum) and the energy of gammaray bursts (GRBs) is explored based on the observed data from BATSE data base (http ://cossc:gsfc:nasa:gov/atse/). Based on a sample of 64 FRED (fast rise and exponential decay) pulse bursts better fitted with the KRL model (refer equation (22) in [1]), it is found that 63, out of the 64 sources, belong to either the platformpower-law-platform feature class or the peaked feature group. The classifications for 64 sources could be sorted into five models in detail: a)a power law range could be observed in 34 sources; b)a lower band platform could be observed or suspected in 18 bursts; c)a higher band platform could be observed or suspected in 7 sources; d)a peaked feature could be observed or suspected in 4 GRBs ;e)the other model from the four types above could be observed in 1 sources .The result suggests that there exists a power law relationship between the pulse FWHM of GRBs and the energy .And the result confirms the points from Qin et al (2005)[2] that the relationship is due to the Doppler effect of fireballs." @default.
- W2463725397 created "2016-07-22" @default.
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- W2463725397 date "2007-03-01" @default.
- W2463725397 modified "2023-10-17" @default.
- W2463725397 title "Revisite of the Energy Dependence on the Pulse Width in Gamma-Ray Bursts" @default.
- W2463725397 hasPublicationYear "2007" @default.
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