中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
VERY HIGH ENERGY gamma-RAY AFTERGLOW EMISSION OF NEARBY GAMMA-RAY BURSTS

文献类型:期刊论文

作者Xue, R. R.1,2; Tam, P. H.3; Wagner, S. J.3; Behera, B.3; Fan, Y. Z.1,4; Wei, D. M.1,5
刊名ASTROPHYSICAL JOURNAL
出版日期2009-09-01
卷号703期号:1页码:60-67
ISSN号0004-637X
关键词gamma rays: bursts ISM: jets and outflows radiation mechanisms: non-thermal
英文摘要The synchrotron self-Compton (SSC) emission from gamma-ray burst (GRB) forward shock can extend to the very high energy (VHE; E gamma > 100 GeV) range. Such high energy photons are rare and are attenuated by the cosmic infrared background before reaching us. In this work, we discuss the prospect to detect these VHE photons using the current ground-based Cherenkov detectors. Our calculated results are consistent with the upper limits obtained with several Cherenkov detectors for GRB 030329, GRB 050509B, and GRB 060505 during the afterglow phase. For five bursts in our nearby GRB sample (except for GRB 030329), current ground-based Cherenkov detectors would not be expected to detect the modeled VHE signal. Only for those very bright and nearby bursts like GRB 030329, detection of VHE photons is possible under favorable observing conditions and a delayed observation time of less than or similar to 10 hr.
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]INVERSE COMPTON EMISSION ; LIGHT CURVES ; HOST GALAXY ; OPTICAL AFTERGLOW ; HESS OBSERVATIONS ; LONG-DURATION ; UPPER LIMITS ; SWIFT ; GRB-030329 ; COMPONENT
收录类别SCI
语种英语
WOS记录号WOS:000269625000007
公开日期2011-12-08
源URL[http://159.226.72.40/handle/332002/1611]  
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, Grad Sch, Beijing 100012, Peoples R China
3.Univ Heidelberg, D-6900 Heidelberg, Germany
4.Univ Copenhagen, Niels Bohr Inst, Niels Bohr Int Acad, DK-2100 Copenhagen, Denmark
5.Nanjing Univ, Purple Mt Observ, Joint Ctr Particle Nucl Phys & Cosmol, Nanjing 210008, Peoples R China
推荐引用方式
GB/T 7714
Xue, R. R.,Tam, P. H.,Wagner, S. J.,et al. VERY HIGH ENERGY gamma-RAY AFTERGLOW EMISSION OF NEARBY GAMMA-RAY BURSTS[J]. ASTROPHYSICAL JOURNAL,2009,703(1):60-67.
APA Xue, R. R.,Tam, P. H.,Wagner, S. J.,Behera, B.,Fan, Y. Z.,&Wei, D. M..(2009).VERY HIGH ENERGY gamma-RAY AFTERGLOW EMISSION OF NEARBY GAMMA-RAY BURSTS.ASTROPHYSICAL JOURNAL,703(1),60-67.
MLA Xue, R. R.,et al."VERY HIGH ENERGY gamma-RAY AFTERGLOW EMISSION OF NEARBY GAMMA-RAY BURSTS".ASTROPHYSICAL JOURNAL 703.1(2009):60-67.

入库方式: OAI收割

来源:紫金山天文台

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