YNAO OpenIR  > 高能天体物理研究组
GRB 081029: A GAMMA-RAY BURST WITH A MULTI-COMPONENT AFTERGLOW
Holland, ST1,2,3; De Pasquale, M4; Mao JR(毛基荣)5,6,7,8; Sakamoto, T1,3,9; Schady, P4,10; Covino, S5; Fan, YZ11; Jin, ZP5,11; D'Avanzo, P5; Antonelli, A12; D'Elia, V12; Chincarini, G5; Fiore, F12; Pandey, SB13,14; Cobb, BE15; Holland, ST (reprint author), NASA, Goddard Space Flight Ctr, Astrophys Sci Div, Code 660-1,8800 Greenbelt Rd, Greenbelt, MD 20771 USA.
发表期刊ASTROPHYSICAL JOURNAL
2012-01-20
卷号745期号:1
DOI10.1088/0004-637X/745/1/41
产权排序第6完成单位
收录类别SCI
关键词Gamma-ray Burst: General Gamma-ray Burst: Individual: Grb 081029
摘要We present an analysis of the unusual optical light curve of the gamma-ray burst GRB 081029, a long-soft burst with a redshift of z = 3.8479. We combine X-ray and optical observations from the Swift X-Ray Telescope and the Swift UltraViolet/Optical Telescope with ground-based optical and infrared data obtained using the REM, ROTSE, and CTIO 1.3 m telescopes to construct a detailed data set extending from 86 s to similar to 100000 s after the BAT trigger. Our data cover a wide energy range from 10 keV to 0.77 eV (1.24 angstrom-16000 angstrom). The X-ray afterglow shows a shallow initial decay followed by a rapid decay starting at about 18000 s. The optical and infrared afterglow, however, shows an uncharacteristic rise at about 3000 s that does not correspond to any feature in the X-ray light curve. Our data are not consistent with synchrotron radiation from a jet interacting with an external medium, a two-component jet, or continuous energy injection from the central engine. We find that the optical light curves can be broadly explained by a collision between two ejecta shells within a two-component jet. A growing number of gamma-ray-burst afterglows are consistent with complex jets, which suggests that some (or all) gamma-ray-burst jets are complex and will require detailed modeling to fully understand them.
项目资助者NASA [NNX08AV63G] ; NSF [PHY-0801007]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-637X
URL查看原文
WOS记录号WOS:000300316600041
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SWIFT ULTRAVIOLET/OPTICAL TELESCOPE ; SPECTRAL IRRADIANCE CALIBRATION ; LIGHT CURVES ; COMMON ORIGIN ; DUST ; REDSHIFT ; JET ; PROMPT ; BAT ; ENVIRONMENT
引用统计
被引频次:16[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5025
专题高能天体物理研究组
中国科学院天体结构与演化重点实验室
通讯作者Holland, ST (reprint author), NASA, Goddard Space Flight Ctr, Astrophys Sci Div, Code 660-1,8800 Greenbelt Rd, Greenbelt, MD 20771 USA.
作者单位1.Astrophysics Science Division, Code 660.1, 8800 Greenbelt Road, Goddard Space Flight Centre, Greenbelt, MD 20771, USA
2.Universities Space Research Association, 10211 Wincopin Circle, Suite 500 Columbia, MD 21044, USA
3.Centre for Research and Exploration in Space Science and Technology, Code 668.8, 8800 Greenbelt Road, Goddard Space Flight Centre, Greenbelt, MD 20771, USA
4.Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking RH5 6NT, UK
5.INAF-Osservatorio Astronomico di Brera, Via Emilio Bianchi 46, I-23807 Merate (LC), Italy
6.Yunnan Observatory, Chinese Academy of Sciences, Kumming, Yunan Province 650011, China
7.International Centre for Astrophysics, Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon, Republic of Korea 305-348
8.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, Yunnan Province 650011, China
9.Joint Centre for Astrophysics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA
10.Max-Planck-Institut für Extraterrestrische Physik, Gießenbachstraße, D-85748 Garching, Germany
11.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
12.INAF-Osservatorio Astronomico di Roma, Via de Frascati 33, I-00040 Monteporzio Catone (Roma), Italy
13.Randall Laboratory of Physics, University of Michigan, 450 Church St, Ann Arbor, MI 48109-1040, USA
14.Aryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital 263129, India
15.Department of Physics, The George Washington University, 725 21st St NW, Washington, DC 20052, USA
推荐引用方式
GB/T 7714
Holland, ST,De Pasquale, M,Mao JR,et al. GRB 081029: A GAMMA-RAY BURST WITH A MULTI-COMPONENT AFTERGLOW[J]. ASTROPHYSICAL JOURNAL,2012,745(1).
APA Holland, ST.,De Pasquale, M.,Mao JR.,Sakamoto, T.,Schady, P.,...&Holland, ST .(2012).GRB 081029: A GAMMA-RAY BURST WITH A MULTI-COMPONENT AFTERGLOW.ASTROPHYSICAL JOURNAL,745(1).
MLA Holland, ST,et al."GRB 081029: A GAMMA-RAY BURST WITH A MULTI-COMPONENT AFTERGLOW".ASTROPHYSICAL JOURNAL 745.1(2012).
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
GRB 081029_ A GAMMA-(881KB)期刊论文作者接受稿开放获取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
[Holland, ST]的文章
[De Pasquale, M]的文章
[Mao JR(毛基荣)]的文章
百度学术
百度学术中相似的文章
[Holland, ST]的文章
[De Pasquale, M]的文章
[Mao JR(毛基荣)]的文章
必应学术
必应学术中相似的文章
[Holland, ST]的文章
[De Pasquale, M]的文章
[Mao JR(毛基荣)]的文章
相关权益政策
暂无数据
收藏/分享
文件名: GRB 081029_ A GAMMA-RAY BURST WITH A MULTI-COMPONENT AFTERGLOW.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。