X-ray flashes from off-axis nonuniform jets | |
Jin, ZP; Wei, DM | |
刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS |
2004-10-01 | |
卷号 | 4期号:5页码:473-480 |
关键词 | X-rays : general gamma rays : bursts ISM : jets and outflows |
ISSN号 | 1009-9271 |
英文摘要 | It has been widely believed that the outflows in gamma-ray bursts are jetted and some jets may have structures like epsilon(theta) proportional to theta(-k). We check the possibility that X-ray flashes come from such jets. Both qualitative and quantitative analyses have shown that this model can reproduce most of the observational features of both X-ray flashes and gamma-ray bursts. Using the usual parameters of gamma-ray bursts, we have carried out numerical calculations for both uniform and nonuniform jets, of their fluxes, spectra and peak energies. It seems that nonuniform jets are more appropriate to these observational properties than uniform jets. We have also shown that in our model the observational ratio of gamma-ray bursts to X-ray flashes is about a few units. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | STANDARD ENERGY RESERVOIR ; AFTERGLOW LIGHT CURVES ; GAMMA-RAY ; BURST AFTERGLOWS ; VIEWING ANGLE ; SPECTRA ; MODEL ; PREDICTIONS ; EVOLUTION ; EMISSION |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000224698100006 |
公开日期 | 2012-12-22 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/7745] |
专题 | 紫金山天文台_宇宙伽马暴、中子星及相关物理研究团组 |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Jin, ZP,Wei, DM. X-ray flashes from off-axis nonuniform jets[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2004,4(5):473-480. |
APA | Jin, ZP,&Wei, DM.(2004).X-ray flashes from off-axis nonuniform jets.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,4(5),473-480. |
MLA | Jin, ZP,et al."X-ray flashes from off-axis nonuniform jets".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 4.5(2004):473-480. |
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