YNAO OpenIR  > 丽江天文观测站(南方基地)
Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts
Bi, Xiongwei1,2; Mao JR(毛基荣)2,3,4; Liu CX(刘传玺)3,4,5; Bai JM(白金明)2,3,4
发表期刊ASTROPHYSICAL JOURNAL
2018-10-20
卷号866期号:2页码:15
DOI10.3847/1538-4357/aadcf8
产权排序第3完成单位
收录类别SCI
关键词Gamma Rays: General Radiation Mechanisms: Non-thermal
摘要

We build a comprehensive sample to statistically describe the properties of X-ray flashes (XRFs) and X-ray riches (XRRs) from the third Swift Burst Alert Telescope (BAT3) catalog of Gamma-ray bursts (GRBs). We obtain 81 XRFs, 540 XRRs, and 394 classical GRBs (C-GRBs). We statistically explore the different properties of the.-ray prompt emission, the X-ray emission, the X-ray light-curve type, the association with supernovae (SNe), and the host galaxy properties for these sources. We confirm that most XRFs/XRRs are long GRBs with low values of peak energy Epeak obs and they are low-luminosity GRBs. XRFs, XRRs, and C-GRBs follow the same EX, iso-E., iso-Epeak, z correlations. Compared to the classical GRBs, XRFs are favorable to have the association with SN explosions. We do not find any significant differences of redshift distribution and host galaxy properties among XRFs, XRRs, and C-GRBs. We also discuss some observational biases and selection effects that may affect our statistical results. The GRB detectors with wide energy range and low energy threshold are expected for the XRF/XRR research in the future.

资助项目National Natural Science Foundation of China[11661161010] ; National Natural Science Foundation of China[11673062] ; Oversea Talent Program of Yunnan Province ; National Natural Science Foundation of China[11433004] ; Open Project Program of the Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201501] ; Scientific Research Foundation of the Education Department of Yunnan Province[2014Y463] ; National Natural Science Foundation of China[11404103] ; Hundred Talent Program ; Major Program of the Chinese Academy of Sciences[KJZD-EW-M06] ; Ministry of Science and Technology of China[2016YFA0400700]
语种英语
学科领域天文学
学科门类理学 ; 理学::天文学
文章类型Article
出版者IOP PUBLISHING LTD
ISSN0004-637X
URL查看原文
WOS记录号WOS:000448150800011
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]Off-axis ; Host Galaxies ; E-p,E-i-e-iso Correlation ; Light Curves ; Grb 130427a ; Jet Models ; Afterglow ; Supernovae ; Universal ; Emission
引用统计
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/18041
专题丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
通讯作者Mao JR(毛基荣)
作者单位1.Department of Physics, Honghe University, 661199 Mengzi, People's Republic of China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, People's Republic of China
3.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, Yunnan Province, People's Republic of China
4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, 100012 Beijing, People's Republic of China
5.University of Chinese Academy of Sciences, 100049 Beijing, People's Republic of China
推荐引用方式
GB/T 7714
Bi, Xiongwei,Mao JR,Liu CX,et al. Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts[J]. ASTROPHYSICAL JOURNAL,2018,866(2):15.
APA Bi, Xiongwei,Mao JR,Liu CX,&Bai JM.(2018).Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts.ASTROPHYSICAL JOURNAL,866(2),15.
MLA Bi, Xiongwei,et al."Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts".ASTROPHYSICAL JOURNAL 866.2(2018):15.
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
Statistical Study of(6715KB)期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Bi, Xiongwei]的文章
[Mao JR(毛基荣)]的文章
[Liu CX(刘传玺)]的文章
百度学术
百度学术中相似的文章
[Bi, Xiongwei]的文章
[Mao JR(毛基荣)]的文章
[Liu CX(刘传玺)]的文章
必应学术
必应学术中相似的文章
[Bi, Xiongwei]的文章
[Mao JR(毛基荣)]的文章
[Liu CX(刘传玺)]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

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。