Multi-wavelength study of MGRO J2019+37

CORC > 高能物理研究所 > 中国科学院高能物理研究所 > 粒子天体物理中心

	Multi-wavelength study of MGRO J2019+37
	Hou C(侯超); Chen SZ(陈松战); Yuan Q(袁强); Hou, C; Chen, SZ; Yuan, Q; Cao, Z; He, HH; Sheng, XD;; Cao Z(曹臻)
刊名	CHINESE PHYSICS C
	2014
卷号	38 期号:8 页码:85001
关键词	MGRO J2019+37 multi-wavelength VHE gamma-ray radiation mechanism
英文摘要	MGRO J2019+37, within the Cygnus region, is a bright extended source revealed by Milagro at 12-35 TeV. This source is almost as bright as the Crab Nebula in the northern sky, but is not confirmed by ARGO-YBJ around the TeV scale. Up to now, no obvious counterpart at low energy wavelengths has been found. Hence, MGRO J2019+37 is a rather mysterious object and its VHE gamma-ray emission mechanism is worth investigating. In this paper, a brief summary of the multi-wavelength observations from radio to gamma-rays is presented. All the available data from XMM-Newton and INTEGRAL at X-ray, and Fermi-LAT at gamma-ray bands, are used to get constraints on its emission flux at low energy wavelengths. Then, its possible counterparts and the VHE emission mechanism are discussed.
学科主题	Physics
收录类别	SCI
WOS记录号	WOS:000340350200007
公开日期	2016-05-03
内容类型	期刊论文
源URL	[http://ir.ihep.ac.cn/handle/311005/224944]
专题	高能物理研究所_粒子天体物理中心
推荐引用方式 GB/T 7714	Hou C,Chen SZ,Yuan Q,et al. Multi-wavelength study of MGRO J2019+37[J]. CHINESE PHYSICS C,2014,38(8):85001.
APA	侯超.,陈松战.,袁强.,Hou, C.,Chen, SZ.,...&盛祥东.(2014).Multi-wavelength study of MGRO J2019+37.CHINESE PHYSICS C,38(8),85001.
MLA	侯超,et al."Multi-wavelength study of MGRO J2019+37".CHINESE PHYSICS C 38.8(2014):85001.