Property Changes of Gamma-Ray Bursts
LI Ti-pei
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039
Property Changes of Gamma-Ray Bursts
LI Ti-pei
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039
关键词 ：
98.70.Rz ,
96.50.Ci ,
98.62.Nx
Abstract ： From analysing the third burst and transient source experiment gamma-ray burst catalog, systematic variations of average observational characteristics of γ-ray bursts (GRBs) with a time scale of months to years are revealed, which raise a difficulty to existing models and indicate an origin of GRBs, at least partly, within the heliosphere. A possible GRB producing process is discussed.
Key words ：
98.70.Rz
96.50.Ci
98.62.Nx
出版日期: 1996-08-01
:
98.70.Rz
(γ-ray sources; γ-ray bursts)
96.50.Ci
(Solar wind plasma; sources of solar wind)
98.62.Nx
(Jets and bursts; galactic winds and fountains)
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[3]
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[4]
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[5]
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[6]
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[7]
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[8]
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[9]
HUANG Yong-Feng;DAI Zi-Gao;LU Tan;. Afterglows from Jetted Gamma-Ray-Burst Remnant: Does the Light Curve Break?
[10]
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[11]
HUANG Yong-feng;DAI Zi-gao;LU Tan;. Overall Evolution of Realistic Gamma-Ray Burst Remnant and Its Afterglow
[12]
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[13]
ZHANG Shu;LI Ti-pei;WU Mei. A Possible Glitch of Gamma-Ray Pulsar Geminga?
[14]
LI Ti-pei;WU Mei. Gamma-Ray Bursts from Discharges in Plasmas
[15]
ZHANG Shu;LI Ti-pei;WU Mei. Compton Telescope Observation of Gamma-Ray Flare from Quasar PKS0528+134
1996, Vol. 13 
