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GRB afterglows: Deep Newtonian phase and its application
Huang, YF; Lu, T; Cheng, KS
2005-05-01
Source PublicationNUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS
Volume28Issue:3Pages:415-418
AbstractGamma-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.
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1393/ncc/i2005-10141-2
WOS KeywordGAMMA-RAY BURSTS ; FIREBALL ; MODEL ; CALORIMETRY ; GRB-030329 ; EVOLUTION ; BEPPOSAX ; EJECTA ; JET
Indexed ByISTP ; SCI
Language英语
WOS Research AreaAstronomy & Astrophysics ; Geochemistry & Geophysics
WOS SubjectAstronomy & Astrophysics ; Geochemistry & Geophysics
WOS IDWOS:000233646000038
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/10956
Collection院士文集_陆埮
Affiliation1.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
GB/T 7714
Huang, YF,Lu, T,Cheng, KS. GRB afterglows: Deep Newtonian phase and its application[J]. NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS,2005,28(3):415-418.
APA Huang, YF,Lu, T,&Cheng, KS.(2005).GRB afterglows: Deep Newtonian phase and its application.NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS,28(3),415-418.
MLA Huang, YF,et al."GRB afterglows: Deep Newtonian phase and its application".NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS 28.3(2005):415-418.
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