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题名: GRB afterglows: Deep Newtonian phase and its application
作者: Huang, YF; Lu Tan(陆埮); Cheng, KS
刊名: NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS
出版日期: 2005-05-01
卷号: 28, 期号:3, 页码:415-418
学科分类: Astronomy & Astrophysics
DOI: 10.1393/ncc/i2005-10141-2
文章类型: Article
英文摘要: Gamma-ray burst afterglows have been observed for months or even years in a few cases. It is worth noting that at such late stages, the remnants should have entered the deep Newtonian phase, during which the majority of shock-accelerated electrons will no longer be highly relativistic. To calculate the afterglows, we must assume that the electrons obey a power law distribution according to their kinetic energy, not simply the Lorentz factor.
WOS标题词: Science & Technology ; Physical Sciences
类目[WOS]: Astronomy & Astrophysics ; Geochemistry & Geophysics
研究领域[WOS]: Astronomy & Astrophysics ; Geochemistry & Geophysics
关键词[WOS]: GAMMA-RAY BURSTS ; FIREBALL ; MODEL ; CALORIMETRY ; GRB-030329 ; EVOLUTION ; BEPPOSAX ; EJECTA ; JET
收录类别: ISTP ; SCI
语种: 英语
WOS记录号: WOS:000233646000038
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/10956
Appears in Collections:陆埮_期刊论文

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作者单位: 1.Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
2.Chinese Acad Sci, Purple Mtn Observ, Nanjing 210008, Peoples R China
3.Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China

Recommended Citation:
黄永锋、陆 埮、郑广生.GRB afterglows: Deep Newtonian phase and its application,Nuovo Cimento,2005,28C(415-418):
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