Relationship between the gamma-ray burst pulse width and energy due to the doppler effect of fireballs | |
Tan YP(覃一平)1,2; Dong YM(董云明)1,3; Lu RJ(陆睿静)1,2,3; Zhang BB(张彬彬)1,3; Jia LW(贾兰伟)1,3; Qin, YP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Yunnan, Peoples R China. | |
发表期刊 | ASTROPHYSICAL JOURNAL |
2005-10-20 | |
卷号 | 632期号:2页码:1008-1020 |
DOI | 10.1086/444408 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Gamma Rays : Bursts Gamma Rays : Theory Relativity |
摘要 | We study in detail how the pulse width of gamma-ray bursts is related to energy under the assumption that the sources concerned are in the fireball stage. Due to the Doppler effect of fireballs, there exists a power-law relationship between the two quantities within a limited range of frequency. The power-law range and power-law index depend strongly on the observed peak energy E-p as well as the rest-frame radiation form, and the upper and lower limits of the power-law range can be determined by Ep. It is found that within the same power-law range, the ratio of the FWHM of the rising portion to that of the decaying phase of the pulses is also related to energy in the form of power laws. A plateau/power law/plateau feature is observed in the two relationships. In the case of an obvious softening of the rest-frame spectrum, the two power-law relationships also exist, but the feature evolves to a peaked one. Predictions of the relationships in the energy range covering both the BATSE and Swift bands for a typical hard burst and a typical soft one are made. A sample of FRED (fast rise and exponential decay) pulse bursts shows that 27 out of the 28 sources belong to either the plateau/power law/ plateau feature class or to the peaked feature group, suggesting that the effect concerned is indeed important for most of the sources of the sample. Among these bursts, many might undergo an obvious softening evolution of the rest- frame spectrum. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-637X |
URL | 查看原文 |
归档日期 | 2005-11-02 |
WOS记录号 | WOS:000232569100030 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | RELATIVISTIC MOTION ; SPECTRAL FEATURES ; TIME PROFILES ; BATSE ; CATALOG ; BRIGHT ; PEAK ; VARIABILITY ; BEPPOSAX ; LOCALIZATION |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6987 |
专题 | 星系研究组 |
通讯作者 | Qin, YP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Yunnan, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming, Yunnan 650011, China 2.Physics Department, Guangxi University, Nanning, Guangxi 530004, China 3.Graduate School of the Chinese Academy of Sciences, P.O. Box 3908, Beijing 100039, China |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Tan YP,Dong YM,Lu RJ,et al. Relationship between the gamma-ray burst pulse width and energy due to the doppler effect of fireballs[J]. ASTROPHYSICAL JOURNAL,2005,632(2):1008-1020. |
APA | Tan YP,Dong YM,Lu RJ,Zhang BB,Jia LW,&Qin, YP .(2005).Relationship between the gamma-ray burst pulse width and energy due to the doppler effect of fireballs.ASTROPHYSICAL JOURNAL,632(2),1008-1020. |
MLA | Tan YP,et al."Relationship between the gamma-ray burst pulse width and energy due to the doppler effect of fireballs".ASTROPHYSICAL JOURNAL 632.2(2005):1008-1020. |
条目包含的文件 | ||||||
文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
Relationship between(1265KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论