VERY HIGH ENERGY gamma-RAY AFTERGLOW EMISSION OF NEARBY GAMMA-RAY BURSTS

CORC > 紫金山天文台 > 中国科学院紫金山天文台 > 宇宙伽马暴、中子星及相关物理研究团组

	VERY HIGH ENERGY gamma-RAY AFTERGLOW EMISSION OF NEARBY GAMMA-RAY BURSTS
	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
	2009-09-01
卷号	703 期号:1 页码:60-67
关键词	gamma rays: bursts ISM: jets and outflows radiation mechanisms: non-thermal
ISSN号	0004-637X
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
内容类型	期刊论文
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.